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 | 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)
Do not touch this parameter! default (keV): ``175 600 1000'' |
IBIS_IP_E_band_max_s | string | List of higher energy boundary (single)
Do not touch this parameter! default (keV): ``600 1000 10000'' |
IBIS_IP_E_band_min_m | string | List of lower energy boundary (multiple)
Do not touch this parameter! default (keV): ``350 600 1000'' |
IBIS_IP_E_band_max_m | string | List of higher energy boundary (multiple)
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 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 events
default: `` '' |
IBIS_SM_inEnergyValues | string | DOL of the energy values for multiple
events
default: `` '' |
IBIS_SP_ChanNum | integer | Number of Channels
possible values: 0 - 300 default: 51 |
IBIS_SP_E_band_min_s | string | List of lower limits of output energy bands (single)
default: `` '' |
IBIS_SP_E_band_max_s | string | List of upper limits of output energy bands (single)
default: `` '' |
IBIS_SP_E_band_min_m | string | List of lower limits of output energy bands (multiple)
default: `` '' |
IBIS_SP_E_band_max_m | string | List of upper limits of output energy bands (multiple)
default: `` '' |
IBIS_SPS_ChanNum | integer | Number of Channels
possible values: -1 - 256 default: -1 |
IBIS_SPS_E_band_min_s | string | List of lower limits of output energy
bands
for SINGLE
default: `` '' |
IBIS_SPS_E_band_max_s | string | List of upper limits of output energy
bands
for SINGLE
default: `` '' |
IBIS_SPS_E_band_min_m | string | List of lower limits of output energy
bands
for multiple
default: `` '' |
IBIS_SPS_E_band_max_m | string | List of upper limits of output energy
bands
for multiple
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" |