| Name | Type | Description |
| ogDOL | string | DOL of the Observational Group to be analyzed.
default: ``'' |
|---|---|---|
| jemxNum | integer | JEM-X instrument number (1 or 2)
default: 2 |
| startLevel | string | Analysis level at which analysis
begins. The names of the possible analysis levels
are listed in the table 4
default: ``COR'' |
| endLevel | string | Analysis level at which
analysis finishes. The names of the possible analysis levels
are listed in the table 4.
default: ``IMA2'' |
| skipLevels | string | Analysis levels to be skipped (use with caution!)
default: ``BKG,LCR,BIN_T'' |
| chatter | integer | Verbosity level
possible values: 0 - 5 2 - normal default: 2 |
| clobber | boolean | Clobber existing output data?
default: y |
| osimData | boolean | Input data was created by ISDC simulator?
default: n |
| ignoreScwErrors | boolean | Ignore all SW processing errors?
default: n |
| skipSPEfirstScw | boolean | Do you want to skip SPE
analysis for SCWs during periods of highly variable gain following
reactivation of the instruments?
default: YES |
| Parameters copied to several binning data tasks | ||
| nChanBins | integer | Number of energy-resolved shadowgrams to create. If
, shadowgrams created in standard bands.
Possible values: -7 - 100 default: 4 |
| chanLow | string | Lower channel boundaries for shadowgrams and lightcurves
default: ``46 83 129 160'' |
| chanHigh | string | Upper channel boundaries for shadowgrams and lightcurves
default: ``82 128 159 223'' |
| timeStart | real | Start of time interval [IJD]
-1 - use Science Window bounds default: -1 |
| timeStop | real | End of time interval [IJD]
-1 - use Science Window bounds default: -1 |
| nPhaseBins | integer | Number of phase bins
(N 0 = abs(N) equally spaced bins) default: 0 |
| phaseBins | string | Phase bin sizes, separated by space
default: |
| radiusLimit | real | Use events within this detector radius [mm]
possible values: 0.0 -130.0 default: 122.0 |
| Parameters required for Instrument Characteristics selection | ||
| IC_Group | string | DOL of the Instrument Characteristics
master group. This group is accessed by the script to find the
calibration data relevant for the current Science Window.
default:"" ``../../idx/ic/ic_master_file.fits[GROUPING,1]'' |
| IC_Alias | string | Selection alias for Instrument
Characteristics. By changing this alias different instances of IC data
can be selected.
default: ``OSA'' |
| instMod | string | DOL of JEM-X Instrument Model Group
(empty=find in IC) default:"" |
| response | string | Filename of standard RMF and ARF
(empty=find in IC) default:"" |
| Parameters specific to corrections (COR) | ||
| COR_gainHist | string | DOL of the Index Group with gain
variation history. This data is stored per revolution and
thus not accessible via the IC system.
default: ``'' |
| COR_gainModel | integer | Gain history smoothing model to be applied
possible values: -1 (default) Let the algorithm choose between the optimal model to be used. 0 Linear interpolation between gain history values, 1 This model is obsolete. 2 Exponential gain decay with linear segment immediately after switch. Models normal time variation of gain in a revolution 3 Non-trigger dependent model. 4 Hardware trigger dependency in the smoothing. If there is no significant trigger variation during the revolution, then the program defaults back to model 3. default: -1 |
| COR_outputExists | boolean | Assume already existing output
default: ``n'' |
| COR_randPos | boolean | Should output positions be randomized within the pixel?
default: ``n'' |
| Parameters specific to Good Time Intervals (GTI) | ||
| GTI_gtiUser | string | DOL of the input user GTI
default: ``'' |
| GTI_TimeFormat | string | Time format to be used
possible values: ``IJD'', ``UTC'', ``OBT'' default: ``IJD'' |
| GTI_BTI_Dol | string | DOL of a bad time interval table.
default: `` '' |
| GTI_BTI_Names | string | Input Bad Time Interval names to be considered
default: ``BAD_RESPONCE BAD_CONFIGURATION'' |
| GTI_attTolerance | real | Accepted attitude variability [arc min]
default: 0.5 |
| GTI_limitTable | string | DOL of table with parameter limits
default: ``'' |
| GTI_gtiJemxNames | string | Names of instrumental GTIs to be
included in merged GTI
default: ``'' |
| GTI_gtiScNames | string | Names of spacecraft GTIs to be
included in merged GTI
default: ``'' |
| GTI_MergedName | string | Name of merged GTI to be used
in analysis
default: ``MERGED'' |
| GTI_Accuracy | string | Used accuracy for OBT to IJD conversion
and vice versa
possible values: ``any'', ``inaccurate'', ``accurate'' default: ``any'' |
| GTI_AttStability_Z | real | Accepted attitude stability tolerance of Z axis [arcmin]
default: ``3.0'' |
| Parameters specific to Dead Time Calculation (DEAD) | ||
| DEAD_outputExists | boolean | Assume already existing output
default: ``n'' |
| Parameters specific to catalog extraction (CAT_I) | ||
| CAT_I_refCat | string | DOL of the Reference Catalog
default: ``$ISDC_REF_CAT'' |
| CAT_I_usrCat | string | DOL of the User Catalog. Currently not used.
default: ``'' |
| CAT_I_radiusMin | string | Low limit for the position
selection. Can be multiple limits with separating blank
default: ``0 2.4'' |
| CAT_I_radiusMax | string | High limit for the position
selection. Can be multiple limits with separating blank
default: ``2.4 5.8'' |
| CAT_I_fluxDef | string | Column used for flux selection.
default: ``0'' |
| CAT_I_fluxMin | string | Low limit for flux selection.
default: ``'' |
| CAT_I_fluxMax | string | High limit for flux selection.
default: ``'' |
| CAT_I_class | string | Object class of sources to select
default: ``'' |
| CAT_I_date | real | IJD for the public data.
possible values: 0 - all public; 0 - all private; 0 - according to DAY_ID default: ``-1'' |
| Parameters specific to shadowgram binning (BIN_I) | ||
| BIN_I_evtType | integer | Event type
possible values: 0 - FULL, 1 - REST, -1 - both default: -1 |
| BIN_I_shdType | integer | Type of shadowgram
possible values: 0 - skew 1 - shadowgram based on corrected event positions 2 - shadowgram based on raw event positions (required for j_ima_iros) 3 - shadowgram based on regularized detector pixels default: 2 |
| BIN_I_shdRes | string | DOL of the output shadowgrams
default: ``'' |
| BIN_I_rowSelect | string | CFITSIO selection string on events. Ensures removal of
all hotspot events and other seriously bad events
default: ``&&STATUS 256&& '' |
| BIN_I_gtiNames | string | Names of GTI tables to be used
default: ``'' |
| BIN_I_chanLowDet | string | Three lower channel boundaries for shadowgrams for source detection
default: `` 46 96 135'' |
| BIN_I_chanHighDet | string | Three upper channel boundaries for shadowgrams for source detection
default: ``95 134 178'' |
| Parameters specific to imaging (IMA) | ||
| IMA_makeNewBPL | boolean | Do you want to create a new backprojection file ?
default: no |
| IMA_newBackProjFile | string | Base name of new backprojection file
default: ``'' |
| IMA_detAccLimit | integer | Acceptance limit in JMXi-DETE-MOD data structure.
Possible values: 1 - 65535
default: 16384 |
| IMA_skyImageDim | integer | Sky image dimension.
Possible values: 1:255, 2:511.
default: 2 |
| IMA_useDeadAnodes | boolean | Do you want to include dead anodes areas ?
default: no |
| IMA_maxNumSources | integer | Max number of sources in IROS loop
default: 10 |
| IMA_edgeEnhanceFactor | real | Edge enhancement factor. It is used to convert
the sky-images to significance maps by amplifying the peaks near the edge relative
to those near the center
default: 1.0 |
| IMA_loopLimitPeak | real | Fractional peak power to stop IROS loop
default: 0.025 |
| IMA_detSigSingle | real | Detection significance for source acceptance
default: 12.0 |
| IMA_skyRadiusFactor | real | Sky radius limit factor
default: 1.0 |
| IMA_radiusLimit0 | real | Detector radius limit E
6 keV (mm)
default: 120.0 |
| IMA_radiusLimit1 | real | Detector radius limit 6
E
12 keV (mm)
default: 120.0 |
| IMA_radiusLimit2 | real | Detector radius limit 12
E
20 keV (mm)
default: 1107.0 |
| IMA_radiusLimit3 | real | Detector radius limit E
20 keV (mm)
default: 110.0 |
| IMA_interactionDepth | real | Mean depth of interaction in the detector (mm)
default: 3.0 |
| IMA_hotPixelLimit | real | Hot pixel limit factor above average
default: 4.0 |
| IMA_skyImagesOut | string | Type of output sky images.
There are the following types:
RECTIFIED: Rectified (cleaned) intensity maps (in counts/cm /s). VARIANCE: Variance maps. RECONSTRUCTED: Reconstructed Residual+Sources maps (in counts/cm /s) which only differ from the RECTIFIED maps if sources have been found. RAWINTENSITY: Raw intensity (strength) maps (in counts), for which the vignetting correction is not applied. RESIDUAL: Intensity map (in counts/cm /s) after all found source contributions have been subtracted PIF: activate the ”PIF-weighted” image generation algorithm (not to be used with mosaic_spec) Only the first five letters are required. default: ``RECONSTRUCTED,VARIANCE'' |
| IMA_dolBPL | string | DOL of backprojection file list
default: ``empty'' |
| IMA_bkgShdDOL | string | DOL of background shadowgrams
default: ``empty'' |
| IMA_relDist | real | Limit of relative distance (mm) to catalog
position used for identifying sources
default: 1.5 |
| IMA_fluxLimit | real | Lower flux limit for alerts of unfound sources [Counts/s
]
default: 0.000 |
| IMA_searchRad | real | Range of search grid around nominal found source positions
default: 5.00 |
| IMA_gridNum | integer | Number of grid steps on one side of search grid
default: 10 |
| IMA_distFuzz | real | 'Fuzz' allowed in relative distances
default: 0.15 |
| IMA_signifLim | integer | Minimum number of pixels to make a contribution to the sky image
default: 25 |
| IMA_illumNorm | integer | Flag for special re-normalization
default: 0 |
| IMA_collHreduc | real | [mm] Reduction of collimator height for BPL production"
default: 0. |
| IMA_detImagesOut | boolean | Should the images used for source detection be in output?
default: NO |
| IMA_userImagesOut | boolean | Do you want the user defined images to be
written?
default: YES |
| Parameters specific to source spectra extraction (SPE) | ||
| SPE_InSourceResult | string | Input source result (JMXi-SRCL-RES)
default: ``'' |
| SPE_OutSourceSpectrum | string | Output source spectra (JMXi-SRCL-SPE)
default: ``'' |
| SPE_OutSourceARF | string | Output source spectra (JMXi-SRCL-ARF)
default: ``'' |
| Parameters specific to source lightcurve extraction (LCR) | ||
| LCR_timeStep | real | Binning time for spectra in
seconds, negative value means that time bin is equal to the
science window exposure.
default: 0.0 |
| LCR_vignCorr | boolean | Correct for vignetting?
Forced to "yes". Vignetting correction is always applied. default: y |
| LCR_evtType | integer | Event type (0=FULL, 1=REST, -1=both)
possible values: 0 - FULL, 1 - REST, -1 - both default: -1 |
| LCR_precisionLevel | integer | Speed - precision level, see more details in Section 8.7.1
possible values: 20 - the only value presently supported. default: 20 |
| LCR_fluxScaling | integer | Flux scaling to area
possible values: 1 - Full area open to the illumination 2 - 100cm 3 - 1cm default: 2 |
| LCR_skipNearDeadAnode | boolean | Ignore pixels near dead anodes?
default: y |
| LCR_skipHotSpot | boolean | Ignore pixels in hotspot area?
default: n |
| LCR_tAccuracy | integer | Time Correlation accuracy
possible values: 0 - high, 1 - low, 3 - any default: 3 |
| LCR_rowSelect | string | CFITSIO selection string on events
default: `` '' |
| LCR_useRaDec | boolean | Use sky coordinates (Ra,Dec) instead of instrument coordinates?
default: y |
| LCR_overrideCollTilt | real | Value of collimator tilt parameter. If
0 use
Instrument Model Group value.
default: -1.0 |
| Parameters specific to detector spectra binning (BIN_S) | ||
| BIN_S_timeStep | real | Binning time [s] for spectra (0.0=bin all data)
default: ``0.0'' |
| BIN_S_rowSelectEvts | string | CFITSIO selection string on events
default: ``'' |
| BIN_S_rowSelectSpec | string | CFITSIO selection string on spectrum mode data
default: ``'' |
| BIN_S_evtType | integer | Data format to bin
possible values: -1 - all, 0 - FULL, 1 - REST, 2 - SPTI, 4 - SPEC default: -1 |
| Parameters specific to detector lightcurve binning (BIN_T) | ||
| BIN_T_rowSelect | string | CFITSIO selection string on events
default: ``'' |
| BIN_T_evtType | integer | Data format to bin
possible values: -1 - all, 0 - FULL, 1 - REST, 2 - SPTI, 4 - SPEC default: -1 |
| Parameters specific to jemx_obs_analysis (IMA_2) | ||
| IMA2_mapSelect | string | Types of images to be selected.
Possible values:
RAW_RECT: Rectified (cleaned) intensity maps (in counts/cm /s). RAW_INT: raw intensity (strength) maps (in counts), for which the vignetting correction should not have been applied at the IMA level (by use of "NOVIGN" in the IMA_skyImagesOut parameter line) but is applied at the mosaicking level. RES+SRC: reconstructed Residual+Sources maps (in counts/cm /s) which only differ from the RAW_RECT maps if sources have been found at the IROS imaging level. default: ``RAW_RECT'' |
| IMA2_radiusSelect | real | Input images selection radius in degrees
default: 4.8 |
| IMA2_eminSelect | real | Minimum energy (keV) to select energy interval
default: 0.0 |
| IMA2_emaxSelect | real | Maximum energy (keV) to select energy interval
default: 80.0 |
| IMA2_diameter | real | Diameter in degrees of the mosaic image
(0: allows to fit the mosaic size from the inputs,
: can be used for larger mosaics)
default: 0.0 |
| IMA2_cdelt | real | Pixel size in degrees at mosaic center
default: 0.026 |
| IMA2_RAcenter | real | Center of the mosaic image Right Ascension in degrees (If
0 use the
computed middle position of the mosaic)
default: -1 |
| IMA2_DECcenter | real | Center of the mosaic image Declination in degrees (not used if RAcenter
0)
default: 0.0 |
| IMA2_outfile | string | Prefix of the mosaic FITS file for each energy band
default: ``'' |
| IMA2_viewTime | boolean | Create total exposure time map?
(if Y
OBS_TIME_n.fits, where n is the number of combined input skymaps)
default: "y" |
| IMA2_viewIntens | boolean | Create raw Intensity map?
default: "y" |
| IMA2_viewVar | boolean | Create Variance map?
default: "y" |
| IMA2_viewSig | boolean | Create Significance map?
default: "y" |
| IMA2_view_nb | boolean | Create a map that shows the number of
input images contributing to each pixel?
default "n" |
| IMA2_dolBPL | string | DOL of the vignetting maps, e.g., ../../ic/jmx1/rsp/jmx1_bpl_grp_0002.fits[JMX1-DMAP-BPL]
default: "" |
| IMA2_print_ScWs | boolean | List input Science Windows in mosaic headers?
default: "n" |
| IMA2_AITproj | boolean | Project map in galactic coordinates using AIToff-Hammer projection
default: "n" |
| IMA2_srcFileDOL | string | DOL of the output source list mosaic
default:"" |
| IMA2_srcselect | string | CFITSIO selection string applied to input tables
default:"" |
| IMA2_srcattach | boolean | Attach resulting table to group?
default: y |