Next: Bibliography Up: Data Analysis in Details Previous: Timing Analysis without the

List of ibis_science_analysis parameters

Table 61: ibis_science_analysis parameters description. Query parameters are marked with bold font.

Name Type Description

General parameters

ogDOL string DOL of the Observational Group to be analyzed.
default: ``og_ibis.fits''

startLevel string Analysis level at which the analysis begins. The names of the possible analysis levels are given in section 5.
Possible values: ``COR'' - ``COMP''. Also ``CLEAN'' value is possible.
default: ``COR''

endLevel string Analysis level at which analysis finishes. The names of the possible analysis levels are given in the section 5.
possible values: COR - CLEAN. We recommend you to proceed by steps, as described in the cookbook.
default: ``IMA2''

staring boolean Enter yes if it was a staring observation. It has an influence on PICsIT analysis - for staring observation all shadowgrams are summed before the deconvolution.
default: no

tolerance real tolerance for staring. In case of staring=yes the check is performed that during the Science Windows within the Observation Group the spacecraft was stable within the given tolerance.
default: 0.1

sum_spectra boolean Do the summing of spectra?
default: ``no''

CAT_refCat string DOL of Reference Catalog
default: ``$ISDC_REF_CAT[ISGRI_FLAG>0]''

CAT_usrCat string DOL of User Catalog (CURRENTLY IGNORED!!!)

chatter integer Verbosity level
possible values: 0 - 5, 0 = errors only, 1 = warnings, 2 = normal, ...
default: 2

IC_Group string DOL of Instrument Characteristics master group
default:
``$REP_BASE_PROD/idx/ic/ic_master_file.fits''

IC_Alias string Selection alias for Instrument Characteristics
default: ``OSA''

corrDol string DOL of the isgri off-axis corrections
default: `` ''

rebinned_corrDol_ima string DOL of the rebinned isgri off-axis corrections for imaging
default: `` ''

rebinned_corrDol_spe string DOL of the rebinned isgri off-axis corrections for spectrum
default: `` ''

rebinned_corrDol_lc string DOL of the rebinned isgri off-axis corrections for lc
default: `` ''

rebinned_backDol_ima string DOL of the rebinned isgri back corrections for imaging
default: `` ''

rebinned_backDol_spe string DOL of the rebinned isgri back corrections for spectrum
default: `` ''

rebinned_backDol_lc string DOL of the rebinned isgri back corrections for lc
default: `` ''

GENERAL_clobber boolean Clobber existing output data?
default: YES

GENERAL_levelList boolean List of all levels
default:
COR,GTI,DEAD,BIN_I,BKG_I,CAT_I,IMA,IMA2,BIN_S,SPE,LCR,COMP,CLEAN

Parameters to define which part of data should be analyzed

SWITCH_disableIsgri boolean Disable ISGRI analysis?
possible values: YES, NO
default: NO

SWITCH_disablePICsIT boolean Disable PICsIT analysis?
possible values: YES, NO
default: YES

SWITCH_disableCompton boolean Disable Compton analysis?
possible values: YES, NO
default: YES

SWITCH_osimData boolean Data are from simulator?
possible values: YES, NO
default: NO

Parameters for ibis binning and ibis image reconstruction

IBIS_II_ChanNum integer Number of output energy bands for ISGRI
possible values: -1 - 10
value -1 is for more than 10 energy bands, in this case IBIS_II_inEnergyValues should be set.
default: 4

IBIS_II_E_band_min string List of lower limits of output energy bands (keV) for ISGRI
default: ``20 40 60 100''

IBIS_II_E_band_max string List of upper limits of output energy bands (keV) for ISGRI
default: ``40 60 100 200''

IBIS_II_inEnergyValues string DOL of the energy values when required.
default: `` ''

IBIS_IPS_corrPDH integer (for PICsIT only) Packets threshold for partially downloaded histograms.
default:0

IBIS_IPS_ChanNum integer Number of Energy bands for PICsIT in standard mode.
possible values: 0 - 256
You should set it to -1 to build automatically the only binning for which background maps are present. It corresponds to the following energy ranges (keV): 203 -252, 252 - 329, 329 - 455, 455 - 655, 655 - 1057, 1057 - 1841, 1841 - 3570, 3570 - 6510.
default: -1

IBIS_IPS_E_band_min_s string List of lower energy boundary for PICsIT in standard mode for SINGLE.
Do not touch this parameter!
default: ''''

IBIS_IPS_E_band_max_s string List of higher energy boundary for PICsIT in standard mode for SINGLE.
Do not touch this parameter!
default: ``''

IBIS_IPS_E_band_min_m string List of lower energy boundary for PICsIT in standard mode for MULTIPLE.
Do not touch this parameter!
default: ``''

IBIS_IPS_E_band_max_m string List of higher energy boundary for PICsIT in standard mode for MULTIPLE.
Do not touch this parameter!
default: ``''

IBIS_IP_ChanNum integer Number of Energy bands for PICsIT in photon-by-photon mode.
possible values: 1 - 300
Do not touch this parameter!
default: 3

IBIS_IP_E_band_min_s string List of lower energy boundary (single) for PICsIT
Do not touch this parameter!
default (keV):
``175 600 1000''

IBIS_IP_E_band_max_s string List of higher energy boundary (single) for PICsIT
Do not touch this parameter!
default (keV):
``600 1000 10000''

IBIS_IP_E_band_min_m string List of lower energy boundary (multiple) for PICsIT
Do not touch this parameter!
default (keV):
``350 600 1000''

IBIS_IP_E_band_max_m string List of higher energy boundary (multiple) for PICsIT
Do not touch this parameter!
default (keV):
``600 1000 13500''

IBIS_NoisyDetMethod integer Noisy Pixel detection method
possible values: 0 (only normal noisy detection), 1 (add also spectral noisy detection)
default: 1

These parameters are recommended by the IBIS team, better not to change them.

IBIS_min_rise integer Minimum rise time.
default: 16

IBIS_max_rise integer Maximum rise time.
default:116

IBIS_P_convFact real Conversion factor channel-to-energy.
default: 7.1

ModPixShad integer Minimum number of non-illuminated pixels per module
possible values: 100 - 500
default:400

Parameters specific to SCW1 pipeline.

SCW1_ISGRI_event_select string CFITSIO event selection string
default: `` ''

SCW1_GTI_LimitTable string DOL of the limit table for GTIs
default: `` ''

SCW1_GTI_attTolerance_X real Accepted attitude stability tolerance of X (optical) axis to generate a GTI [arc min]
possible values: 0 - 10800
default: 0.5

SCW1_GTI_attTolerance_Z real Accepted attitude stability tolerance of Z axis to generate a GTI [arc min]"
possible values: 0 - 10800
default: 3.0

SCW1_GTI_gtiUserP string DOL of the user GTI table for PICsIT
default: `` ''

SCW1_GTI_gtiUserI string DOL of the user GTI table for ISGRI
default: `` ''

SCW1_GTI_TimeFormat string Time format to be used
possible values: ``IJD'', ``UTC'', ``OBT''
default: ``IJD''

SCW1_GTI_Accuracy string Used accuracy for OBT to IJD conversion and vice versa
possible values: ``any'', ``inaccurate'', ``accurate''
default: ``any''

SCW1_GTI_SCP string Names of spacecraft GTIs to be merged for PICsIT
default: `` ''

SCW1_GTI_SCI string Names of spacecraft GTIs to be merged for ISGRI
default: `` ''

SCW1_GTI_PICsIT string GTIs to be merged for PICsIT
default:
``VETO ATTITUDE P_SGLE_DATA_GAPS P_MULE_DATA_GAPS''

SCW1_GTI_ISGRI string GTIs to be merged for ISGRI
default: ``VETO ATTITUDE ISGRI_DATA_GAPS''

SCW1_GTI_BTI_Dol string DOL of a bad time interval table (GNRL-INTL-BTI)
default: ``IBIS_CONFIGURATION IBIS_BOOT ISGRI_RISE_TIME VETO_PROBLEM SOLAR_FLARE BELT_CROSSING''

SCW1_GTI_BTI_Names string Input BTI names to be considered
default: `` ''

SCW1_ICOR_idxSwitch string DOL of the index of pixels switches list.
default: `` ''

SCW1_ICOR_GODOL string DOL of the gain-offset table
default: `` ''

SCW1_ICOR_supGDOL string DOL of gain coefficients for 2nd method
default: `` ''

SCW1_ICOR_supODOL string DOL of offset coefficients for 2nd method"
default: `` ''

SCW1_ICOR_riseDOL string DOL of the rise time correction table
default: `` ''

switDOL string switch on time
default: `` ''

SCW1_ICOR_rtcDOL string rise time correction
default: `` ''

SCW1_RTdriftCor integer RT correction level increasing from 0 to 2.If 0, no RT correction, 2 RT drift included into corrections, 1 default value
default: 1

SCW1_ICOR_probShot real Probability of shot time decay.
default: 0.0001

SCW1_PCOR_enerDOL string DOL of the energy correction table (PICsIT)
default: `` ''

SCW1_BIN_cleanTrk integer Cleaning of cosmic-ray induced events.
possible values:
0 = No
1 = Yes
default: 1

SCW1_veto_mod string DOL of the IC file for VETO model and width of Compton window
default: `` ''

SCW1_BIN_I_idxNoisy string DOL of the index of noisy maps.
default: `` ''

SCW1_BIN_I_idxLowThre string index of Low Threshold
default: `` ''

SCW1_BIN_P_inDead string DOL of the dead time data structure.
default: `` ''

SCW1_BIN_P_inGTI string DOL of the good time interval data structure.
default: `` ''

SCW1_BIN_P_PicsCxt string DOL of the PICsIT Context Tables.
default: `` ''

SCW1_BIN_P_HepiLut string DOL of the hepi lut
default: `` ''

SCW1_BKG_divide boolean Divide by efficiency? Do not touch it!
default: no

SCW1_BKG_badpix boolean Remove bad pixels? Do not touch it!
default: yes

SCW1_BKG_flatmodule boolean flatten modules? Do not touch it!
default: no

SCW1_BKG_I_isgrUnifDol string DOL of the ISGRI detector uniformity
possible values:
DOL for a specific model
``-'' - no uniformity correction
`` '' - DOL is taken from the IC tree
default: ``-''

SCW1_BKG_I_isgrBkgDol string DOL of the ISGRI background model
possible values:
DOL for a specific model
``-'' - no background subtraction
`` '' - DOL is taken from the IC tree
default: `` ''

SCW1_BKG_I_method_cor integer Method to be applied for background removal
possible values:
0 - no background correction
1 - background from IC tree is applied to the whole detector
2 - background is threaded for each module separately
When using 1 or 2, brPif and brPifThreshold parameters are taken into account.
default: ``1''

brSrcDOL string DOL of the bright sources catalogue, which will be removed from background mean calculation
default: ``$ISDC_REF_CAT[ISGRI_FLAG>0&&ISGR_FLUX_1>100]''

SCW1_BKG_I_brPifThreshold real pixels with PIF value higher will be removed from background calculation.
When = 1, bright PIF removal will not be performed
possible values: ``0 - 1 ''
default: ``0.0001''

SCW1_BKG_I_pif string filename of the pif in every ScW
default: `` ''

SCW1_BKG_I_method_int integer Method to be applied for the pixel value interpolation
possible values:
0 - pixels in dead zones are filled with zeros
1 - pixels are filled with mean detector value
default: ``1''

tungAtt string DOL of the Tungsten attenuation length fits file
default: `` ''

aluAtt string DOL of the Aluminium attenuation length fits file
default: `` ''

leadAtt string DOL of the Lead attenuation length fits file
default: `` ''

SCW1_BKG_P_method integer Method applied in filling gaps
possible values:
0 - model (in cts) is normalized by the time of observation
1 - model (in cts) is normalized by the mean count value
default: 0

SCW1_BKG_picsSUnifDOL string DOL of the PICsIT Detector Uniformity model (single).
default: ``-''

SCW1_BKG_picsSBkgDOL string DOL of the PICsIT Detector Background model (single).
default: `` ''

SCW1_BKG_picsMUnifDOL string DOL of the PICsIT Detector Uniformity model (multiple).
default: ``-''

SCW1_BKG_picsMBkgDOL string DOL of the PICsIT Detector Background model (multiple).
default: `` ''

Parameters specific to OBS1 pipeline.

ii_skyimage parameters

OBS1_DataMode integer Data Simulation mode
possible values:
0 - shadowgrams are treated
1 - shadowgrams are simulated
default: 0

rebin_slope real Spectral slope to be used
default: -2

rebin_arfDol string DOL of the ISGRI arf for rebinning.
default: `` ''

OBS1_SearchMode integer Source search mode
possible values for the Science Window analysis:
1 - search for all catalog sources
2 - search for K sources,where K= ToSearch
3 - search for all catalog sources plus for K significant excesses,where K = ToSearch
For all the above, when the mosaic is created, the software looks for K = ToSearch sources.
default: 3

OBS1_ToSearch integer Number of sources to be looked for
default: 50

OBS1_CleanMode integer Ghost cleaning
possible values:
1 - source model lobes are subtracted from the deconvolved image
-1 - no subtraction
default: 1

OBS1_ExtenType integer Save exposure/residual maps
possible values: absent, 0 - 3,
0 or absent - no action
1 - true exposure maps are saved in 4*n extension of isgri_sky_ima.fits instead of residual images
2 - true exposure maps are saved in the 5*n extension of isgri_sky_ima.fits after the residual images
3 - one true exposure map is created for the last energy band and saved in the last extension of isgri_sky_ima.fits
default: 2

OBS1_NegModels integer 0 or absent for no negative models ; 1 - negative models
default: 0

OBS1_FastOpen integer if 1 then no CommonPreparePars
default: 1

ISGRI_mask string DOL of the MASK pattern fits file
default: `` ''

OBS1_deco string DOL of the projected decoding pattern fits file
default: `` ''

OBS1_covrMod string DOL of the covariance fits file
default: ``''

OBS1_ScwType string Type of Science Window to be treated
possible values: ``POINTING'', ``SLEW'', ``OTHER'', ``ANY''
default: ``POINTING''

OBS1_DoPart2 integer if 1 or absent do mosaic part.
Set it to 0 if don't want to produce a mosaic image.
Set it to 2 if you want to produce a mosaic image from different existing runs.
default: 1

OBS1_MapAlpha real Mosaic map center [deg]
default: ""

OBS1_MapDelta real Mosaic map center [deg]
default: ""

OBS1_MapSize real Mosaic map radius [deg]
default: 40.0

OBS1_PixSpread integer 0 - no flux spread in mosaic
default: 1

OBS1_MinCatSouSnr real The software detects a catalog source only if its signal-to-noise ratio is higher than this value.
default: 6

OBS1_MinNewSouSnr real The software detects a catalog source only if its signal-to-noise ratio is higher than this value.
default: 7

OBS1_SouFit integer defines whether to fit or not the source position
0 - for fitting source position in ScW fit
1 - for fixed source position in ScW fit
default: 0

PICSIT_detThr real Detection Threshold
default: 3.0

PICSIT_inCorVar integer Corrected variance to be used [0=NO; 1=YES]
default: 1

PICSIT_outVarian integer Variance maps in output [0=NO; 1=YES]
default: 0

cat_extract parameters, see Section 12.7 for more details.

OBS1_CAT_radiusMin string Low limit for the position selection.
default: ``0''

OBS1_CAT_radiusMax string High limit for the position selection.
default: ``20''

OBS1_CAT_fluxDef string Column used for flux selection.
default: `` ''

OBS1_CAT_fluxMin string Low limit for flux selection.
default: `` ''

OBS1_CAT_fluxMax string High limit for flux selection.
default: `` ''

OBS1_CAT_class string Select the object by class.
default: `` ''

OBS1_CAT_date real IJD for the public data.
default: 1

Parameters specific to SCW2 pipeline.

PICSIT_deco string DOL of the MASK decoding fits file
default: `` ''

SCW2_cat_for_extract string Catalog for spectral and lightcurve extraction
(if empty then it is taken from the imaging result of the Science Window)
default: `` ''

SCW2_racolumn string Name of the column where to get Ra
default: ``RA_FIN''

SCW2_deccolumn string Name of the column where to get Dec
default: ``DEC_FIN''

SCW2_catalog string Catalog for PICsIT imaging
default: `` ''

SCW2_PIF_filter string filter to apply on the source
default: `` ''

SCW2_ISGRI_event_select string CFITSIO event selection string
default: `` ''

parameter for building light curves from PICsIT spectral timing data

Parameters for spectra extraction.

IBIS_SI_ChanNum integer Number of Channels
possible values: -1 - 10,
-1 = take from ISGR-EBDS-MOD structure. In this case parameter IBIS_SI_inEnergyValues must contain the DOL of the rebinned matrix.
default: -1

IBIS_SI_E_band_min string List of lower limits of output energy bands
default: `` ''

IBIS_SI_E_band_max string List of upper limits of output energy bands
default: `` ''

IBIS_SI_inEnergyValues string DOL of the energy values when required.
default: `` ''

PICSIT_source_name string Name of the source for extracting PICsIT spectrum
default: `` ''

PICSIT_source_RA real RA of the source for extracting PICsIT spectrum
default: `` ''

PICSIT_source_DEC real DEC of the source for extracting PICsIT spectrum
default: `` ''

IBIS_SS_inEnergyValues string DOL of the energy values for single PICsIT events
default: `` ''

IBIS_SM_inEnergyValues string DOL of the energy values for multiple PICsIT events
default: `` ''

IBIS_SP_ChanNum integer Number of Channels for PICsIT
possible values: 0 - 300
default: 51

IBIS_SP_E_band_min_s string List of lower limits of output energy bands (PICsIT single events)
default: `` ''

IBIS_SP_E_band_max_s string List of upper limits of output energy bands (PICsIT single events)
default: `` ''

IBIS_SP_E_band_min_m string List of lower limits of output energy bands (PICsIT multiple events)
default: `` ''

IBIS_SP_E_band_max_m string List of upper limits of output energy bands (PICsIT multiple events)
default: `` ''

IBIS_SPS_ChanNum integer Number of Channels for PICsIT
possible values: -1 - 256
default: -1

IBIS_SPS_E_band_min_s string List of lower limits of output energy bands for SINGLE PICsIT events
default: `` ''

IBIS_SPS_E_band_max_s string List of upper limits of output energy bands for SINGLE PICsIT events
default: `` ''

IBIS_SPS_E_band_min_m string List of lower limits of output energy bands for multiple PICsIT events
default: `` ''

IBIS_SPS_E_band_max_m string List of upper limits of output energy bands for multiple PICsIT events
default: `` ''

SCW2_ISPE_idx_isgrResp string DOL of the index of ISGRI response matrices
default: ``''

SCW2_ISPE_isgrarf string DOL of the ARFs for XSPEC
default: ``''

SCW2_ISPE_DataMode integer Data Simulation mode
default: 0

SCW2_ISPE_MethodInt integer Method to be applied for the pixel value interpolation
default: 1

SCW2_ISPE_MethodFit integer Method to be applied for background and source intensity fitting
default: 6

SCW2_ISPE_isgrUnifDol string DOL of the ISGRI detector uniformity
default: ``''

SCW2_BIN_cleanTrk integer Cleaning of cosmic-ray induced events.
possible values:
0 = No
1 = Yes
default: 0

SCW2_BIN_I_idxNoisy string DOL of the index of noisy maps.
default: ``''

SCW2_BIN_I_idxLowThre string index of Low Threshold
default: ``''

SCW2_BIN_P_inDead string DOL of the dead time data structure.
default: ``''

SCW2_BIN_P_inGTI string DOL of the good time interval data structure.
default: ``''

SCW2_BIN_P_PicsCxt string DOL of the PICsIT Context Tables.
default: `` ''

SCW2_BIN_P_HepiLut string DOL of the hepi lut
default: ``''

SCW2_BKG_I_isgrBkgDol string DOL of the isgri bckg model or - if you want none or empty if you want DOL automatic from the IC tree
default: ``''

SCW2_BKG_divide boolean Divide by efficiency
default: no

SCW2_BKG_badpix boolean Remove bad pixels
default: yes

SCW2_BKG_flatmodule boolean flatten modules
default: no

SCW2_BKG_I_method_cor string Method to be applied for background removal
possible values:
0 - background from IC tree is applied to the whole detector
1 - parameter switches to this value automatically when background map is specified (not an IC one)
2 - background is threaded for each module separately
When using 1 or 2, brPif and brPifThreshold parameters are taken into account.
default: ``2''

SCW2_BKG_I_method_int string Method to be applied for the pixel value interpolation
possible values:
0 - pixels in dead zones are filled with zeros
1 - pixels are filled with mean detector value
default: ``1''

SCW2_BKG_P_method integer Method applied in filling gaps
possible values: 0 - 2
default: 1

SCW2_BKG_picsSUnifDOL string DOL of the PICsIT Detector Uniformity model (single).
default: ``''

SCW2_BKG_picsSBkgDOL string DOL of the PICsIT Detector Background model (single).
default: ``-''

SCW2_BKG_picsMUnifDOL string DOL of the PICsIT Detector Uniformity model (multiple).
default: ``''

SCW2_BKG_picsMBkgDOL string DOL of the PICsIT Detector Background model (multiple).
default: ``-''

Parameters for lightcurve extraction.

ILCR_select string Event selection condition
default: ``''

ILCR_delta_t real Time bin in seconds.
possible values: 0.1 - 10000
default: 100

ILCR_num_e integer Number of energy channels
possible values: 1 - 10
default: 4

ILCR_e_min string List of low energy boundaries
default: ``20 40 60 100''

ILCR_e_max string List of high energy boundaries
default: ``40 60 100 200''

Parameters for PICsIT mosaic extraction.

OBS2_detThr real Detection Threshold (in sigmas).
default: 3.0

OBS2_projSel string Selection of projection
default: STG

OBS2_imgSel string Selection criteria of images.
default: "EVT_TYPE=='SINGLE' && E_MIN==252 && E_MAX==336"

**Table 61:** *ibis_science_analysis* parameters description. Query parameters are marked with bold font.


Name	Type	Description

General parameters
ogDOL	string	DOL of the Observational Group to be analyzed. default: ``og_ibis.fits''

startLevel	string	Analysis level at which the analysis begins. The names of the possible analysis levels are given in section 5. Possible values: ``COR'' - ``COMP''. Also ``CLEAN'' value is possible. default: ``COR''

endLevel	string	Analysis level at which analysis finishes. The names of the possible analysis levels are given in the section 5. possible values: `COR` - `CLEAN`. We recommend you to proceed by steps, as described in the cookbook. default: ```IMA2`''

staring	boolean	Enter `yes` if it was a staring observation. It has an influence on PICsIT analysis - for staring observation all shadowgrams are summed before the deconvolution. default: `no`

tolerance	real	tolerance for staring. In case of staring=`yes` the check is performed that during the Science Windows within the Observation Group the spacecraft was stable within the given tolerance. default: `0.1`

sum_spectra	boolean	Do the summing of spectra? default: ```no`''

CAT_refCat	string	DOL of Reference Catalog default: ``$ISDC_REF_CAT[ISGRI_FLAG>0]''

CAT_usrCat	string	DOL of User Catalog (CURRENTLY IGNORED!!!)

chatter	integer	Verbosity level possible values: `0` - `5`, `0` = errors only, `1` = warnings, `2` = normal, ... default: `2`

IC_Group	string	DOL of Instrument Characteristics master group default: ``$REP_BASE_PROD/idx/ic/ic_master_file.fits''

IC_Alias	string	Selection alias for Instrument Characteristics default: ``OSA''

corrDol	string	DOL of the isgri off-axis corrections default: `` ''

rebinned_corrDol_ima	string	DOL of the rebinned isgri off-axis corrections for imaging default: `` ''

rebinned_corrDol_spe	string	DOL of the rebinned isgri off-axis corrections for spectrum default: `` ''

rebinned_corrDol_lc	string	DOL of the rebinned isgri off-axis corrections for lc default: `` ''

rebinned_backDol_ima	string	DOL of the rebinned isgri back corrections for imaging default: `` ''

rebinned_backDol_spe	string	DOL of the rebinned isgri back corrections for spectrum default: `` ''

rebinned_backDol_lc	string	DOL of the rebinned isgri back corrections for lc default: `` ''

GENERAL_clobber	boolean	Clobber existing output data? default: `YES`

GENERAL_levelList	boolean	List of all levels default: `COR,GTI,DEAD,BIN_I,BKG_I,CAT_I,IMA,IMA2,BIN_S,SPE,LCR,COMP,CLEAN`

Parameters to define which part of data should be analyzed
SWITCH_disableIsgri	boolean	Disable ISGRI analysis? possible values: `YES, NO` default: `NO`

SWITCH_disablePICsIT	boolean	Disable PICsIT analysis? possible values: `YES, NO` default: `YES`

SWITCH_disableCompton	boolean	Disable Compton analysis? possible values: `YES, NO` default: `YES`

SWITCH_osimData	boolean	Data are from simulator? possible values: `YES, NO` default: `NO`

Parameters for ibis binning and ibis image reconstruction
IBIS_II_ChanNum	integer	Number of output energy bands for ISGRI possible values: `-1` - `10` value `-1` is for more than 10 energy bands, in this case `IBIS_II_inEnergyValues` should be set. default: `4`

IBIS_II_E_band_min	string	List of lower limits of output energy bands (keV) for ISGRI default: ``20 40 60 100''

IBIS_II_E_band_max	string	List of upper limits of output energy bands (keV) for ISGRI default: ``40 60 100 200''

IBIS_II_inEnergyValues	string	DOL of the energy values when required. default: `` ''

IBIS_IPS_corrPDH	integer	(for PICsIT only) Packets threshold for partially downloaded histograms. default:`0`

IBIS_IPS_ChanNum	integer	Number of Energy bands for PICsIT in standard mode. possible values: `0` - `256` You should set it to `-1` to build automatically the only binning for which background maps are present. It corresponds to the following energy ranges (keV): 203 -252, 252 - 329, 329 - 455, 455 - 655, 655 - 1057, 1057 - 1841, 1841 - 3570, 3570 - 6510. default: `-1`

IBIS_IPS_E_band_min_s	string	List of lower energy boundary for PICsIT in standard mode for SINGLE. Do not touch this parameter! default: ''''

IBIS_IPS_E_band_max_s	string	List of higher energy boundary for PICsIT in standard mode for SINGLE. Do not touch this parameter! default: ``''

IBIS_IPS_E_band_min_m	string	List of lower energy boundary for PICsIT in standard mode for MULTIPLE. Do not touch this parameter! default: ``''

IBIS_IPS_E_band_max_m	string	List of higher energy boundary for PICsIT in standard mode for MULTIPLE. Do not touch this parameter! default: ``''

IBIS_IP_ChanNum	integer	Number of Energy bands for PICsIT in photon-by-photon mode. possible values: `1` - `300` Do not touch this parameter! default: `3`

IBIS_IP_E_band_min_s	string	List of lower energy boundary (single) for PICsIT Do not touch this parameter! default (keV): ``175 600 1000''

IBIS_IP_E_band_max_s	string	List of higher energy boundary (single) for PICsIT Do not touch this parameter! default (keV): ``600 1000 10000''

IBIS_IP_E_band_min_m	string	List of lower energy boundary (multiple) for PICsIT Do not touch this parameter! default (keV): ``350 600 1000''

IBIS_IP_E_band_max_m	string	List of higher energy boundary (multiple) for PICsIT Do not touch this parameter! default (keV): ``600 1000 13500''

IBIS_NoisyDetMethod	integer	Noisy Pixel detection method possible values: `0` (only normal noisy detection), `1` (add also spectral noisy detection) default: `1`

These parameters are recommended by the IBIS team, better not to change them.
IBIS_min_rise	integer	Minimum rise time. default: `16`

IBIS_max_rise	integer	Maximum rise time. default:`116`

IBIS_P_convFact	real	Conversion factor channel-to-energy. default: `7.1`

ModPixShad	integer	Minimum number of non-illuminated pixels per module possible values: `100 - 500` default:`400`

Parameters specific to SCW1 pipeline.
SCW1_ISGRI_event_select	string	CFITSIO event selection string default: `` ''

SCW1_GTI_LimitTable	string	DOL of the limit table for GTIs default: `` ''

SCW1_GTI_attTolerance_X	real	Accepted attitude stability tolerance of X (optical) axis to generate a GTI [arc min] possible values: `0` - `10800` default: `0.5`

SCW1_GTI_attTolerance_Z	real	Accepted attitude stability tolerance of Z axis to generate a GTI [arc min]" possible values: `0` - `10800` default: `3.0`

SCW1_GTI_gtiUserP	string	DOL of the user GTI table for PICsIT default: `` ''

SCW1_GTI_gtiUserI	string	DOL of the user GTI table for ISGRI default: `` ''

SCW1_GTI_TimeFormat	string	Time format to be used possible values: ``IJD'', ``UTC'', ``OBT'' default: ``IJD''

SCW1_GTI_Accuracy	string	Used accuracy for OBT to IJD conversion and vice versa possible values: ``any'', ``inaccurate'', ``accurate'' default: ``any''

SCW1_GTI_SCP	string	Names of spacecraft GTIs to be merged for PICsIT default: `` ''

SCW1_GTI_SCI	string	Names of spacecraft GTIs to be merged for ISGRI default: `` ''

SCW1_GTI_PICsIT	string	GTIs to be merged for PICsIT default: ``VETO ATTITUDE P_SGLE_DATA_GAPS P_MULE_DATA_GAPS''

SCW1_GTI_ISGRI	string	GTIs to be merged for ISGRI default: ``VETO ATTITUDE ISGRI_DATA_GAPS''

SCW1_GTI_BTI_Dol	string	DOL of a bad time interval table (GNRL-INTL-BTI) default: ``IBIS_CONFIGURATION IBIS_BOOT ISGRI_RISE_TIME VETO_PROBLEM SOLAR_FLARE BELT_CROSSING''

SCW1_GTI_BTI_Names	string	Input BTI names to be considered default: `` ''

SCW1_ICOR_idxSwitch	string	DOL of the index of pixels switches list. default: `` ''

SCW1_ICOR_GODOL	string	DOL of the gain-offset table default: `` ''

SCW1_ICOR_supGDOL	string	DOL of gain coefficients for 2nd method default: `` ''

SCW1_ICOR_supODOL	string	DOL of offset coefficients for 2nd method" default: `` ''

SCW1_ICOR_riseDOL	string	DOL of the rise time correction table default: `` ''

switDOL	string	switch on time default: `` ''

SCW1_ICOR_rtcDOL	string	rise time correction default: `` ''

SCW1_RTdriftCor	integer	RT correction level increasing from 0 to 2.If 0, no RT correction, 2 RT drift included into corrections, 1 default value default: `1`

SCW1_ICOR_probShot	real	Probability of shot time decay. default: `0.0001`

SCW1_PCOR_enerDOL	string	DOL of the energy correction table (PICsIT) default: `` ''

SCW1_BIN_cleanTrk	integer	Cleaning of cosmic-ray induced events. possible values: `0` = No `1` = Yes default: `1`

SCW1_veto_mod	string	DOL of the IC file for VETO model and width of Compton window default: `` ''

SCW1_BIN_I_idxNoisy	string	DOL of the index of noisy maps. default: `` ''

SCW1_BIN_I_idxLowThre	string	index of Low Threshold default: `` ''

SCW1_BIN_P_inDead	string	DOL of the dead time data structure. default: `` ''

SCW1_BIN_P_inGTI	string	DOL of the good time interval data structure. default: `` ''

SCW1_BIN_P_PicsCxt	string	DOL of the PICsIT Context Tables. default: `` ''

SCW1_BIN_P_HepiLut	string	DOL of the hepi lut default: `` ''

SCW1_BKG_divide	boolean	Divide by efficiency? Do not touch it! default: `no`

SCW1_BKG_badpix	boolean	Remove bad pixels? Do not touch it! default: `yes`

SCW1_BKG_flatmodule	boolean	flatten modules? Do not touch it! default: `no`

SCW1_BKG_I_isgrUnifDol	string	DOL of the ISGRI detector uniformity possible values: DOL for a specific model ``-'' - no uniformity correction `` '' - DOL is taken from the IC tree default: ``-''

SCW1_BKG_I_isgrBkgDol	string	DOL of the ISGRI background model possible values: DOL for a specific model ``-'' - no background subtraction `` '' - DOL is taken from the IC tree default: `` ''

SCW1_BKG_I_method_cor	integer	Method to be applied for background removal possible values: `0` - no background correction `1` - background from IC tree is applied to the whole detector `2` - background is threaded for each module separately When using 1 or 2, `brPif` and `brPifThreshold` parameters are taken into account. default: ``1''

brSrcDOL	string	DOL of the bright sources catalogue, which will be removed from background mean calculation default: ``$ISDC_REF_CAT[ISGRI_FLAG>0&&ISGR_FLUX_1>100]''

SCW1_BKG_I_brPifThreshold	real	pixels with PIF value higher will be removed from background calculation. When = 1, bright PIF removal will not be performed possible values: ``0 - 1 '' default: ``0.0001''

SCW1_BKG_I_pif	string	filename of the pif in every ScW default: `` ''

SCW1_BKG_I_method_int	integer	Method to be applied for the pixel value interpolation possible values: `0` - pixels in dead zones are filled with zeros `1` - pixels are filled with mean detector value default: ``1''

tungAtt	string	DOL of the Tungsten attenuation length fits file default: `` ''

aluAtt	string	DOL of the Aluminium attenuation length fits file default: `` ''

leadAtt	string	DOL of the Lead attenuation length fits file default: `` ''

SCW1_BKG_P_method	integer	Method applied in filling gaps possible values: `0` - model (in cts) is normalized by the time of observation `1` - model (in cts) is normalized by the mean count value default: `0`

SCW1_BKG_picsSUnifDOL	string	DOL of the PICsIT Detector Uniformity model (single). default: ``-''

SCW1_BKG_picsSBkgDOL	string	DOL of the PICsIT Detector Background model (single). default: `` ''

SCW1_BKG_picsMUnifDOL	string	DOL of the PICsIT Detector Uniformity model (multiple). default: ``-''

SCW1_BKG_picsMBkgDOL	string	DOL of the PICsIT Detector Background model (multiple). default: `` ''

Parameters specific to OBS1 pipeline.
`ii_skyimage` parameters
OBS1_DataMode	integer	Data Simulation mode possible values: `0` - shadowgrams are treated `1` - shadowgrams are simulated default: `0`

rebin_slope	real	Spectral slope to be used default: `-2`

rebin_arfDol	string	DOL of the ISGRI arf for rebinning. default: `` ''

OBS1_SearchMode	integer	Source search mode possible values for the Science Window analysis: `1` - search for all catalog sources `2` - search for K sources,where K= ToSearch `3` - search for all catalog sources plus for K significant excesses,where K = ToSearch For all the above, when the mosaic is created, the software looks for K = ToSearch sources. default: `3`

OBS1_ToSearch	integer	Number of sources to be looked for default: `50`

OBS1_CleanMode	integer	Ghost cleaning possible values: `1` - source model lobes are subtracted from the deconvolved image `-1` - no subtraction default: `1`

OBS1_ExtenType	integer	Save exposure/residual maps possible values: `absent`, `0` - `3`, `0` or `absent` - no action `1` - true exposure maps are saved in 4n extension of isgri_sky_ima.fits instead of residual images `2` - true exposure maps are saved in the 5n extension of isgri_sky_ima.fits after the residual images `3` - one true exposure map is created for the last energy band and saved in the last extension of isgri_sky_ima.fits default: `2`

OBS1_NegModels	integer	0 or absent for no negative models ; 1 - negative models default: `0`

OBS1_FastOpen	integer	if 1 then no CommonPreparePars default: `1`

ISGRI_mask	string	DOL of the MASK pattern fits file default: `` ''

OBS1_deco	string	DOL of the projected decoding pattern fits file default: `` ''

OBS1_covrMod	string	DOL of the covariance fits file default: ``''

OBS1_ScwType	string	Type of Science Window to be treated possible values: ``POINTING'', ``SLEW'', ``OTHER'', ``ANY'' default: ``POINTING''

OBS1_DoPart2	integer	if `1` or absent do mosaic part. Set it to `0` if don't want to produce a mosaic image. Set it to `2` if you want to produce a mosaic image from different existing runs. default: `1`

OBS1_MapAlpha	real	Mosaic map center [deg] default: `""`

OBS1_MapDelta	real	Mosaic map center [deg] default: `""`

OBS1_MapSize	real	Mosaic map radius [deg] default: `40.0`

OBS1_PixSpread	integer	`0` - no flux spread in mosaic default: `1`

OBS1_MinCatSouSnr	real	The software detects a catalog source only if its signal-to-noise ratio is higher than this value. default: `6`

OBS1_MinNewSouSnr	real	The software detects a catalog source only if its signal-to-noise ratio is higher than this value. default: `7`

OBS1_SouFit	integer	defines whether to fit or not the source position `0` - for fitting source position in ScW fit `1` - for fixed source position in ScW fit default: `0`

PICSIT_detThr	real	Detection Threshold default: `3.0`

PICSIT_inCorVar	integer	Corrected variance to be used [0=NO; 1=YES] default: `1`

PICSIT_outVarian	integer	Variance maps in output [0=NO; 1=YES] default: `0`

cat_extract parameters, see Section 12.7 for more details.
OBS1_CAT_radiusMin	string	Low limit for the position selection. default: ``0''

OBS1_CAT_radiusMax	string	High limit for the position selection. default: ``20''

OBS1_CAT_fluxDef	string	Column used for flux selection. default: `` ''

OBS1_CAT_fluxMin	string	Low limit for flux selection. default: `` ''

OBS1_CAT_fluxMax	string	High limit for flux selection. default: `` ''

OBS1_CAT_class	string	Select the object by class. default: `` ''

OBS1_CAT_date	real	IJD for the public data. default: `1`

Parameters specific to SCW2 pipeline.
PICSIT_deco	string	DOL of the MASK decoding fits file default: `` ''

SCW2_cat_for_extract	string	Catalog for spectral and lightcurve extraction (if empty then it is taken from the imaging result of the Science Window) default: `` ''

SCW2_racolumn	string	Name of the column where to get Ra default: ``RA_FIN''

SCW2_deccolumn	string	Name of the column where to get Dec default: ``DEC_FIN''

SCW2_catalog	string	Catalog for PICsIT imaging default: `` ''

SCW2_PIF_filter	string	filter to apply on the source default: `` ''

SCW2_ISGRI_event_select	string	CFITSIO event selection string default: `` ''

parameter for building light curves from PICsIT spectral timing data
Parameters for spectra extraction.
IBIS_SI_ChanNum	integer	Number of Channels possible values: `-1` - `10`, `-1` = take from ISGR-EBDS-MOD structure. In this case parameter IBIS_SI_inEnergyValues must contain the DOL of the rebinned matrix. default: `-1`

IBIS_SI_E_band_min	string	List of lower limits of output energy bands default: `` ''

IBIS_SI_E_band_max	string	List of upper limits of output energy bands default: `` ''

IBIS_SI_inEnergyValues	string	DOL of the energy values when required. default: `` ''

PICSIT_source_name	string	Name of the source for extracting PICsIT spectrum default: `` ''

PICSIT_source_RA	real	RA of the source for extracting PICsIT spectrum default: `` ''

PICSIT_source_DEC	real	DEC of the source for extracting PICsIT spectrum default: `` ''

IBIS_SS_inEnergyValues	string	DOL of the energy values for single PICsIT events default: `` ''

IBIS_SM_inEnergyValues	string	DOL of the energy values for multiple PICsIT events default: `` ''

IBIS_SP_ChanNum	integer	Number of Channels for PICsIT possible values: `0` - `300` default: `51`

IBIS_SP_E_band_min_s	string	List of lower limits of output energy bands (PICsIT single events) default: `` ''

IBIS_SP_E_band_max_s	string	List of upper limits of output energy bands (PICsIT single events) default: `` ''

IBIS_SP_E_band_min_m	string	List of lower limits of output energy bands (PICsIT multiple events) default: `` ''

IBIS_SP_E_band_max_m	string	List of upper limits of output energy bands (PICsIT multiple events) default: `` ''

IBIS_SPS_ChanNum	integer	Number of Channels for PICsIT possible values: `-1` - `256` default: `-1`

IBIS_SPS_E_band_min_s	string	List of lower limits of output energy bands for SINGLE PICsIT events default: `` ''

IBIS_SPS_E_band_max_s	string	List of upper limits of output energy bands for SINGLE PICsIT events default: `` ''

IBIS_SPS_E_band_min_m	string	List of lower limits of output energy bands for multiple PICsIT events default: `` ''

IBIS_SPS_E_band_max_m	string	List of upper limits of output energy bands for multiple PICsIT events default: `` ''

SCW2_ISPE_idx_isgrResp	string	DOL of the index of ISGRI response matrices default: ``''

SCW2_ISPE_isgrarf	string	DOL of the ARFs for XSPEC default: ``''

SCW2_ISPE_DataMode	integer	Data Simulation mode default: `0`

SCW2_ISPE_MethodInt	integer	Method to be applied for the pixel value interpolation default: `1`

SCW2_ISPE_MethodFit	integer	Method to be applied for background and source intensity fitting default: `6`

SCW2_ISPE_isgrUnifDol	string	DOL of the ISGRI detector uniformity default: ``''

SCW2_BIN_cleanTrk	integer	Cleaning of cosmic-ray induced events. possible values: `0` = No `1` = Yes default: `0`

SCW2_BIN_I_idxNoisy	string	DOL of the index of noisy maps. default: ``''

SCW2_BIN_I_idxLowThre	string	index of Low Threshold default: ``''

SCW2_BIN_P_inDead	string	DOL of the dead time data structure. default: ``''

SCW2_BIN_P_inGTI	string	DOL of the good time interval data structure. default: ``''

SCW2_BIN_P_PicsCxt	string	DOL of the PICsIT Context Tables. default: `` ''

SCW2_BIN_P_HepiLut	string	DOL of the hepi lut default: ``''

SCW2_BKG_I_isgrBkgDol	string	DOL of the isgri bckg model or - if you want none or empty if you want DOL automatic from the IC tree default: ``''

SCW2_BKG_divide	boolean	Divide by efficiency default: `no`

SCW2_BKG_badpix	boolean	Remove bad pixels default: `yes`

SCW2_BKG_flatmodule	boolean	flatten modules default: `no`

SCW2_BKG_I_method_cor	string	Method to be applied for background removal possible values: `0` - background from IC tree is applied to the whole detector `1` - parameter switches to this value automatically when background map is specified (not an IC one) `2` - background is threaded for each module separately When using 1 or 2, `brPif` and `brPifThreshold` parameters are taken into account. default: ``2''

SCW2_BKG_I_method_int	string	Method to be applied for the pixel value interpolation possible values: `0` - pixels in dead zones are filled with zeros `1` - pixels are filled with mean detector value default: ``1''

SCW2_BKG_P_method	integer	Method applied in filling gaps possible values: `0` - `2` default: `1`

SCW2_BKG_picsSUnifDOL	string	DOL of the PICsIT Detector Uniformity model (single). default: ``''

SCW2_BKG_picsSBkgDOL	string	DOL of the PICsIT Detector Background model (single). default: ``-''

SCW2_BKG_picsMUnifDOL	string	DOL of the PICsIT Detector Uniformity model (multiple). default: ``''

SCW2_BKG_picsMBkgDOL	string	DOL of the PICsIT Detector Background model (multiple). default: ``-''

Parameters for lightcurve extraction.
ILCR_select	string	Event selection condition default: ``''

ILCR_delta_t	real	Time bin in seconds. possible values: `0.1` - `10000` default: `100`

ILCR_num_e	integer	Number of energy channels possible values: `1` - `10` default: `4`

ILCR_e_min	string	List of low energy boundaries default: ```20 40 60 100`''

ILCR_e_max	string	List of high energy boundaries default: ```40 60 100 200`''

Parameters for PICsIT mosaic extraction.
OBS2_detThr	real	Detection Threshold (in sigmas). default: `3.0`

OBS2_projSel	string	Selection of projection default: `STG`

OBS2_imgSel	string	Selection criteria of images. default: `"EVT_TYPE=='SINGLE' && E_MIN==252 && E_MAX==336"`

Next: Bibliography Up: Data Analysis in Details Previous: Timing Analysis without the

2018-11-20