| Parameter | Mand | Type | Default | Constraints |
| removetemporaries | no | b | true | yes |
| Remove temporary data sets? | ||||
| removeintermediategtis | no | b | true | yes |
| Remove intermediate GTI data sets? | ||||
| removeintermediateeventlists | no | b | true | yes |
| Remove the intermediate CCD/node-based event lists? | ||||
| withdefaultcal | no | boolean | Y | Y/N |
| whether mode-dependent
calibration-related settings should be used automatically, this will use for:
BURST: withrdpha=“N”, withxrlcorrection=“Y”, runepreject=“Y”, runepfast=“Y” TIMING: withrdpha=“Y”, withxrlcorrection=“Y”, runepreject=“Y”, runepfast=“N” IMAGING: withrdpha=“N”, withxrlcorrection=“N”, runepreject as user-supplied, runepfast=“N” | ||||
| selectccds | no | b | false | yes |
| Select the CCDs to process? false = process all CCDs. | ||||
| ccd1 | no | b | false | yes |
| Process data for CCD 1? | ||||
| ccd2 | no | b | false | yes |
| Process data for CCD 2? | ||||
| ccd3 | no | b | false | yes |
| Process data for CCD 3? | ||||
| ccd4 | no | b | false | yes |
| Process data for CCD 4? | ||||
| ccd5 | no | b | false | yes |
| Process data for CCD 5? | ||||
| ccd6 | no | b | false | yes |
| Process data for CCD 6? | ||||
| ccd7 | no | b | false | yes |
| Process data for CCD 7? | ||||
| ccd8 | no | b | false | yes |
| Process data for CCD 8? | ||||
| ccd9 | no | b | false | yes |
| Process data for CCD 9? | ||||
| ccd10 | no | b | false | yes |
| Process data for CCD 10? | ||||
| ccd11 | no | b | false | yes |
| Process data for CCD 11? | ||||
| ccd12 | no | b | false | yes |
| Process data for CCD 12? | ||||
| selectmodes | no | b | true | yes |
| Select the modes to process? false = process only imaging. | ||||
| imaging | no | b | true | yes |
| Process imaging mode exposure? | ||||
| timing | no | b | true | yes |
| Process timing mode exposures? | ||||
| burst | no | b | false | yes |
| process burst mode exposures? | ||||
| timingsrcposition | no | i | 190 | |
| Source position for TIMING and BURST modes in RAWY pixel coordinates. [Used in epframes.] | ||||
| withinstexpids | no | b | false | yes |
| Select exposures to process? | ||||
| instexpids | no | S | ||
| List of exposures (ie, PNU002) | ||||
| withgtiset | no | b | false | yes |
| Use an external GTI dataset to be used when filtering the data? | ||||
| gtiset | no | e | gti.ds | |
| Name of the external GTI dataset to be used when filtering the data. | ||||
| runhkgtigen | no | b | false | yes |
| Generate a GTI dataset based on housekeeping? | ||||
| runatthkgen | no | b | true | yes |
| Pre-process attitude data through atthkgen? | ||||
| referencepointing | no | s | median | nominal|object|mean|median|user |
| Coordinates of the reference poiting used for the calculation of the sky coordinates | ||||
| ra | no | u | 0.0 | |
| User-specified right ascension of s/c attitude (deg) | ||||
| dec | no | u | 0.0 | |
| User-specified declination of s/c attitude (deg) | ||||
| posangle | no | u | 0.0 | |
| User-specified astronomical position angle of s/c attitude (deg) | ||||
| filterevents | no | b | true | yes |
| Filter the event lists? | ||||
| filterexpression | no | s | ||
| Bad events selection expression. | ||||
| flagfilteredevents | no | b | false | yes |
| Flag the events that match the filter expression instead of removing them? | ||||
| rungtimerge | no | b | no | yes |
| Merge GTIs from each CCD | ||||
| applygti | no | b | true | yes |
| Apply GTI filter to the event lists? | ||||
| runevlistcomb | no | b | true | yes |
| Merge CCD-level event lists into exposure-level event lists (by mode)? | ||||
| othertables | no | list of uppercase strings | BADPIX EXPOSURE STDGTI DLIMAP HKAUX:q! | none |
| names of secondary tables or arrays to propagate | ||||
| deleteexposurecolumns | no | b | true | yes |
| | ||||
| searchforbadpixels | no | b | yes | yes |
| Search for bad pixels? | ||||
| searchforbadcolumns | no | b | yes | yes |
| Look for bad columns? | ||||
| thresholdlabel | no | s | rate | peak|rate|counts |
| Thresholds choice - as percentage of PEAK, as count RATE or pure COUNTS [!badpixfind] | ||||
| lothresh | no | r | 0.0 | |
| Low threshold to search for dead pixels [badpixfind] | ||||
| hithresh | no | r | 0.0045 | |
| High threshold to search for hot pixels [!badpixfind] | ||||
| columnsearchlabel | no | s | median | median|total |
| Columnsearch thresholds choice - refer to TOTAL column value or MEDIAN column value [badpixfind] | ||||
| locolthresh | no | r | 0.0 | |
| Low threshold to search for dead columns [badpixfind] | ||||
| hicolthresh | no | r | 0.00105 | |
| High threshold to search for hot columns [!badpixfind] | ||||
| flickertimesteps | no | i | 1 | |
| Number of timesteps to search for flickering pixels [badpixfind] | ||||
| flickerksthresh | no | r | 0.55 | |
| K-S threshold for low count flickering pixels [badpixfind] | ||||
| flickerchisqthresh | no | r | 15.0 | |
| Reduced Chi-sq threshold for high count flickering pixels [badpixfind] | ||||
| backgroundrate | no | r | 0.0001 | none |
| Background rate (ct/s/pix) - if negative, mean over entire field assumed [!badpixfind] | ||||
| narrowerthanpsf | no | r | 1.5 | |
| PSF-pixel(s) comparison - 1:equal to PSF, >1:more compact [!badpixfind] | ||||
| threshabovebackground | no | b | no | yes |
| High thresholds as values above background [badpixfind] | ||||
| loenergythresh | no | r | 0.14 | |
| Low energy threshold for searching (keV) [!badpixfind] | ||||
| hienergythresh | no | r | 10 | |
| Hi energy threshold for searching (keV) [!badpixfind] | ||||
| randomizeposition | no | b | yes | yes |
| Randomize DETX/DETY within one CCD pixel [epevents] | ||||
| randomizeenergy | no | b | yes | yes |
| Randomize PHA within one ADU bin [epevents] | ||||
| testenergywidth | no | b | yes | yes |
| Use an energy width of 1eV [epevents] | ||||
| gainctiaccuracy | no | i | 2 | |
| Accuracy of gain/cti correction [epevents] | ||||
| reemissionthresh | no | i | none | |
| Re-emission trigger threshold [epevents] | ||||
| withoutoftime | no | b | no | yes |
| Perform out-of-time events analysis instead (Y/N) [epevents] | ||||
| mappatterntype | no | s | sssd | |
| pattern types of the bands for photon maps [!epevents] | ||||
| patternanalysis | no | boolean | Y | Y/N |
|
no, if pattern recognition has been done already (future development)[!epevents] | ||||
| withframecti | no | boolean | N | Y/N |
|
yes, if TIME-derived frame numbers should be used in CTI correction for
non-imaging modes (TI, BU) instead of the ODF frame numbers. For
FF, eFF, LW, SW modes internally always the TIME-derived frame numbers
instead of the dummy ODF numbers are used
(should not be changed). [!epevents]
| ||||
| withpatternoffset | no | boolean | Y | Y/N |
| epevents:
yes, if pattern energy offset corrections should be applied
| ||||
| withbackgroundgain | no | boolean | Y | Y/N |
| epevents:
yes, if background gain corrections should be applied
| ||||
| ctilongtermsoft | no | boolean | Y | Y/N |
| epevents:
special soft energy function
| ||||
| withrdpha | no | boolean | Y | Y/N |
|
yes, if a correction for rate-dependent PHA effects for TI and BU modes
should be applied. The logical keyword PHA_RDCO indicates whether
this correction has been applied or not. If applied, then the keyword
PHA_RDCB gives the scaling factor B used in the correction,
derived from block RDPHA_DERIV in the CTI.CCF. [!epevents]
| ||||
| rdphatimebinsize | no | boolean | 100 | |
|
time-bin size for rate-dependent PHA correction for TI and BU modes [s] [!epevents]
| ||||
| checksasmip | no | boolean | N | Y/N |
| epevents:
yes, if the MIP rejection information obtained by task epframes
shall be printed (only meaningful if on-board rejection is switched off,
i.e. for SW, TI, BU modes).[!epevents]
| ||||
| backgroundtres | no | boolean | N | Y/N |
| epevents:
yes, if averaged discarded line value (rather than time resolved)
shall be used for background gain corrections
| ||||
| backgroundtbin | no | real | 100.0 | 0-150000 |
| epevents:
time bin for averaging time-resolved background level data
| ||||
| wrongpixlimit | no | i | 20 | |
| Allowed percentage of wrong pixels without producing a warning [!epframes] | ||||
| withsrccoords | no | b | no | yes |
| Use user-supplied RA,DEC coordinates for TIMING and BURST mode ? [epframes] | ||||
| srcra | no | u | 0.0 | |
| User-supplied source position RA [deg] [epframes] | ||||
| srcdec | no | u | 0.0 | |
| User-supplied source position DEC [deg] [epframes] | ||||
| mipthreshold | no | i | 3000 | |
| maximum PHA for non-MIPs [epframes] | ||||
| mipmethod | no | s | onboard | none|onboard|com|sas |
| method to reject MIPs [epframes] | ||||
| mipdist | no | b | no | yes |
| Create MIPDIST columns and MIPHIST extension in output (yes/no) ? [epframes] | ||||
| mipdiscard | no | b | yes | yes |
| discard MIPs from event list (yes/no) ? [epframes] | ||||
| setupbpx | no | string | nom6 | cal4/nom0/nom1/ nom2/nom3/nom4/ nom5/nom6/none |
|
setup for badpix/offset correction vector (used only if ccfok=N) [epframes] | ||||
| lowerthreshold | no | integer | 20 | 0-4095 |
| disregard low-energy
events (with amplitudes | ||||
| guessdeltap | no | boolean | N | Y,N |
| whether to estimate the shift of the
PN oscillator frequency due to temperature and ageing effects from HK data,
could be used to estimate SAS_JUMP_TOLERANCE (divide by 6).[epframes] | ||||
| withparameters | no | b | false | yes |
| Specify explicit list of HK parameters? [hkgtigen] | ||||
| parameters | no | S | ||
| List of HK parameters to consider [hkgtigen] | ||||
| except | no | b | false | yes |
| Consider all parameters except those specified [hkgtigen] | ||||
| withoverrideparameters | no | b | false | yes |
| Specify list of additional parameters? [hkgtigen] | ||||
| overrideparameters | no | S | ||
| List of override/additional parameters [hkgtigen] | ||||
| runepnoise | no | b | no | yes |
| Run epnoise task | ||||
| sigmacut | no | real | 3.0 | |
| Sigma cut for bright sources | ||||
| noisecut | no | int | 2 | |
| Noise cut (maximum allowed number of soft events in frame) | ||||
| savemasks | no | boolean | no | yes|no |
| Save CCDs mask to a file | ||||
| runepreject | no | b | no | yes |
| Run epreject task. | ||||
| badcolumnset | no | dataset | badcolumns.tab | |
| Name of optional
ascii file containing pairs of <ccd nr.> <bad column nr.> (one per
line), to be omitted from the offset correction [epreject] | ||||
| sigma | no | real | 4.0 | |
| Sigma threshold for offset correction [epreject] | ||||
| withnoisehandling | no | boolean | no | |
| enables noise flagging scheme [epreject] | ||||
| noiseparameters | no | real | 0.98 12 | |
| Noise fraction parameters (cutoff parameter and 12 chip specific correction factors; only for expert use) [epreject] | ||||
| withoffsetmap | no | boolean | yes | |
| enables use of offset map to calculate energy shifts [epreject] | ||||
| withxrlcorrection | no | boolean | no | |
| turns on X-ray loading correction code for TI+BU modes, only meaningful if offset
maps are availbale in the ODF and use of offset map is not switched off. [epreject] | ||||
| withsoftflarescreening | no | boolean | no | |
| enables soft flare screening (TI mode) [epreject] | ||||
| softflarethreshold1 | no | real | 10.0 | |
| threshold for flare screening in units of counts/0.1 s [epreject] | ||||
| softflarethreshold2 | no | real | 1.0 | |
| threshold for flare screening [epreject] | ||||
| softflaresmooth | no | string | BOX | |
| smoothing method for flare screening [epreject] | ||||
| softflareenergyrange | no | list of int | 40 50 | |
| energy range for flare screening (in ADU units) [epreject] | ||||
| softflaresmoothparams | no | list of real | 2 1 1 | |
| smoothing parameters [epreject] | ||||
| runepexposure | no | b | yes | yes |
| Run epreject task | ||||
| runepxrlcorr | no | b | no | yes |
| Run epxrlcorr task | ||||
| runepfast | no | b | no | yes |
| Run epfast task | ||||
| analyzingSciSimdata | no | S | ||
| Set up the configuration to analyze SciSim data with epproc | ||||
| Parameter | Mand | Type | Default | Constraints |
XMM-Newton SOC -- 2025-01-27