configuration_sim_telarray#
LSTN-01#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
300 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
20 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
LSTN-02#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
300 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
20 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
LSTN-03#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
300 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
20 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
LSTN-04#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
300 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
20 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
LSTS-01#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
300 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
20 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
LSTS-02#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
300 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
20 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
LSTS-03#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
300 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
20 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
LSTS-04#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
300 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
20 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-01#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-02#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-03#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-04#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-05#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-06#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-07#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-08#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-09#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-10#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-11#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-12#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-13#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-14#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTN-15#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-01#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-02#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-03#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-04#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-05#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-06#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-07#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-08#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-09#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-10#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-11#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-12#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-13#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-14#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-15#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-16#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-17#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-18#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-19#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-20#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-21#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-22#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-23#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-24#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTS-25#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTx-FlashCam#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photoelectrons |
1.0.0 |
25 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
min photons |
1.0.0 |
360 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
store photoelectrons |
1.0.0 |
22 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
tailcut scale |
1.0.0 |
2.6 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
MSTx-NectarCam#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photoelectrons |
1.0.0 |
30 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
min photons |
1.0.0 |
450 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
store photoelectrons |
1.0.0 |
26 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
tailcut scale |
1.0.0 |
2.3 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-01#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-02#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-03#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-04#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-05#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-06#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-07#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-08#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-09#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-10#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-11#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-12#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-13#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-14#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-15#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-16#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-17#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-18#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-19#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-20#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-21#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-22#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-23#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-24#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-25#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-26#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-27#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-28#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-29#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-30#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-31#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-32#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-33#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-34#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-35#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-36#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-37#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-38#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-39#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-40#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-41#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-42#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-43#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-44#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-45#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-46#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-47#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-48#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-49#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |
SSTS-50#
Parameter Name |
Parameter Version |
Values |
Short Description |
---|---|---|---|
correct nsb spectrum to telescope altitude |
1.0.0 |
Correct the night-sky background spectrum to the telescope altitude from the altitude where the Benn & Ellison spectrum was measured. The correction is done within sim_telarray and is based on the atmospheric transmission to 2200 m a.s.l (atm_trans_2200_1_3_0_0_0.dat). |
|
iobuf maximum |
1.0.0 |
1000000000 byte |
Buffer limits for input and output of eventio data. |
iobuf output maximum |
1.0.0 |
400000000 byte |
The maximum size of the I/O buffer for output data, including raw data for all telescopes. |
min photoelectrons |
1.0.0 |
12 |
Minimum number of detected photoelectrons required before running electronics simulation. |
min photons |
1.0.0 |
250 |
Minimum number of photons required before doing simulation. |
random generator |
1.0.0 |
mt19937 |
Random generator used. |
sampled output |
1.0.0 |
True |
Select a specific output format (if several available). A value of 0 means to write ADC sums, a value of 1 to write ADC samples. |
save_pe with amplitude |
1.0.0 |
True |
True if photo-electron data is to be stored with the resulting amplitudes (in mean-p.e. units) in addition to the arrival times. Storing of photo-electron data should be activated separately (see save_photons (bit 1) and store_photoelectrons parameters) but non-zero values of this parameter will also activate save_photons bit 1. Storing p.e. in internal calibration events is controlled separately by save_calibration_pe. |
store photoelectrons |
1.0.0 |
10 |
While the save_photons=2 configuration option will save photo-electron data for all events, this parameter allows to set a lower limit on the number of photo-electrons which must get registered before deciding to store them. Setting it to a value of zero or bigger (default: -1) will automatically enable the corresponding save_photons bit. It should be cross-checked that the min_photons parameter is unlikely to result in fewer than the given number of photo- electrons, as no attempt is made to trace photons through the telescope and produce any photo-electrons if there are too few photons in the first place. |
tailcut scale |
1.0.0 |
1 |
The special scheme for selecting pixels belonging to a shower image as implemented in sim_telarray (as opposed to the traditional two-level tailcut scheme) has multiple thresholds for the various levels of confidence that a pixel actually belongs to the shower image. Instead of making them individually configurable, a common scale factor can be applied to all of them. |