XMM-Newton Science Analysis System


rgsproc (rgsproc-1.34.3) [xmmsas_20160201_1833-15.0.0]

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Parameters

This section documents the parameters recognized by this task (if any).

Parameter	Mand	Type	Default	Constraints
entrystage (global)	no	choice	1:events	1:events $\mid\,$ 2:angles $\mid\,$ 3:filter $\mid\,$ 4:spectra $\mid\,$ 5:fluxing $\mid\,$ 6:lightcurve
The stage at which to begin processing.
finalstage (global)	no	choice	5:fluxing	1:events $\mid\,$ 2:angles $\mid\,$ 3:filter $\mid\,$ 4:spectra $\mid\,$ 5:fluxing $\mid\,$ 6:lightcurve
The last stage to process.
withinstexpids (global)	no	boolean	false
On true: only the specified list of exposures (parameter instexpids) are processed. On false: all Spectroscopy exposures are processed.
instexpids (global)	no	list of strings
List of instrument-exposure identifiers. These take two possible forms: a six-character string such as ``R1S001'' or the full name of any ODF file related to the desired exposure. Requires withinstexpids=true.
orders (global)	no	list of integers	1 2	$1 \le integer \le 6$
Which reflection orders to process in the final two stages (``spectra'' and ``fluxing'').
withprefix (global)	no	boolean	false
A prefix string begins the name of every file written to or read from the current working directory. On true: the specified prefix string (parameter prefix) is enabled. On false: the PPS prefix string is inferred from the ODF.
prefix (global)	no	string
Filename prefix string used in the current working directory. Requires withprefix=true.
expunge (global)	no	list of choices	events	events $\mid\,$ merged
Which intermediate datasets may be deleted automatically.
spectrumbinning	no	choice	lambda	lambda beta
Spectrum binning type. Used to accumulate exposure maps and spectrum. Also used to calculate regions
timestep (Stage1/atthkgen)	no	real	1	$real \ge 0$
Time resolution in seconds on which to construct the spacecraft attitude time-series file.
driftlimit (Stage1/attfilter)	no	real	5	$real \ge 0$
Threshold in arc minutes for filtering out time intervals in which the spacecraft attitude drifted too far from the median.
onlylastatt (Stage1/attfilter)	no	boolean	false
If true only the last attitude points (100) are taken for calculating (median) the reference attitude for filtering.
calcoffsets (Stage1/rgsoffsetcalc)	no	boolean	false
The energy calibrations require pulse-height offsets from the CCF. Override values for these can be computed from the diagnostic data. On true: offset overrides are computed and passed to rgsenergy. On false: offset overrides are not computed.
withoffsethistogram (Stage1/rgsoffsetcalc)	no	boolean	false
On true: the pulse-height distributions from the offset computation are written to an output dataset. On false: the distributions are discarded. Requires calcoffsets=true.
withepicset (Stage1/rgssources)	no	boolean	false
On true: suitable entries from the specified EPIC catalog of detected sources (parameter epicset) are added to the output SRCLIST table. On false: no EPIC sources are added.
epicset (Stage1/rgssources)	no	dataset
An EPIC source list, such as produced by tasks emldetect and eboxdetect. Requires withepicset=true.
withsrc (Stage1/rgssources)	no	boolean	false
On true: the specified source (parameters srclabel, etc.) is added to the output SRCLIST table and is established as the primary source for subsequent analyses. On false: there is no user-defined source and so rgssources selects a primary source on its own, giving preference to the Observation Proposal.
srclabel (Stage1/rgssources)	no	string	USER
User-defined source: LABEL column value. This is the name of the source; ideally it should be meaningful and convenient. Requires withsrc=true.
srcrate (Stage1/rgssources)	no	real		$real \ge 0$
User-defined source: RATE column value. This is the RGS band brightness of the source in counts per second, and is used to compute relative confusion between the sources. Requires withsrc=true.
srcstyle (Stage1/rgssources)	no	choice	radec	radec $\mid\,$ wrtatt
User-defined source: this parameter specifies how the source position is to be defined. radec: celestial coordinates (parameters srcra and srcdec). wrtatt: RGS angular coordinates (parameters srcdisp and srcxdsp). This choice is made persistent through the FIXED_ON_SKY column (set true for celestial coordinates) so that subsequent changes to the reference spacecraft attitude affect the derived coordinates but not the defining coordinates. Requires withsrc=true.
srcra (Stage1/rgssources)	no	real	-999
User-defined source: RA column value. This is the right ascension in decimal degrees. Mandatory when applicable. Requires srcstyle=radec.
srcdec (Stage1/rgssources)	no	real	-999
User-defined source: DEC column value. This is the declination in decimal degrees. Mandatory when applicable. Requires srcstyle=radec.
srcdisp (Stage1/rgssources)	no	real
User-defined source: DELTA_DISP column value. This is the dispersion-direction offset from the pointing axis, in arc minutes. Requires srcstyle=wrtatt.
srcxdsp (Stage1/rgssources)	no	real
User-defined source: DELTA_XDSP column value. This is the cross-dispersion-direction offset from the pointing axis, in arc minutes. Requires srcstyle=wrtatt.
attstyle (Stage1/rgssources)	no	choice	expmedian	expmedian $\mid\,$ start $\mid\,$ user
Specifies the method to use for defining the reference spacecraft attitude (pointing of the instrument). expmedian: calculated from the attitude time-series file. start: start-of-exposure attitude as given in the ODF. user: enables the specified attitude (parameters attra, attdec and attapos).
attra (Stage1/rgssources)	no	real	-999
User-defined attitude: right ascension in decimal degrees. Mandatory when applicable. Requires attstyle=user.
attdec (Stage1/rgssources)	no	real	-999
User-defined attitude: declination in decimal degrees. Mandatory when applicable. Requires attstyle=user.
attapos (Stage1/rgssources)	no	real	-999
User-defined attitude: position angle in decimal degrees. Mandatory when applicable. Requires attstyle=user.
withdiagoffset (Stage1/rgsenergy)	no	boolean	false
On true: files included in the ODF (from 2004 on) contain averages of diagnostic images over three consecutive orbits around the data. They are used in this case for an offset subtraction pixel by pixel.
withgain (Stage1/rgsenergy)	no	boolean	true
On true: calibration of the telemetered energy values includes the gain correction. On false: gain correction is not performed.
withcti (Stage1/rgsenergy)	no	boolean	true
On true: calibration of the telemetered energy values includes the CTI correction. On false: CTI correction is not performed.
keepcool	no	boolean	yes
If set to "no", columns showing often larger CTI will be flagged (taken also from the CCF).
withadvisory (Stage1/rgsbadpix)	no	boolean	true
The BADPIXnn tables are a compilation of all known bad pixel locations. The choice of how to use this information to filter the data is not made until the third stage of processing (``filter''). On true: advisory (non-uplinked) bad pixels from the CCF are included. On false: no advisory bad pixels.
withfoundhot (Stage1/rgsbadpix)	no	boolean	true
On true: the telemetry is analyzed for pixels that appear to be hot (frequently yielding spurious detections) according to criteria set by the following parameters. Any such pixel locations are then included in the BADPIXnn tables. On false: hot pixel finding is disabled. Not applicable to HTR mode data.
pixnoiselimit (Stage1/rgsbadpix)	no	integer		$0 \le integer \le 4095$
Hot pixel finding: lowest uncalibrated single-pixel energy to be considered. Requires withfoundhot=true.
pixsharpness (Stage1/rgsbadpix)	no	real	5	$real \ge 0$
Hot pixel finding: sharpness criterion (see rgsbadpix documentation). Requires withfoundhot=true.
colnoiselimit (Stage1/rgsbadpix)	no	integer	250	$0 \le integer \le 4095$
Hot column finding: lowest uncalibrated single-pixel energy to be considered. Requires withfoundhot=true.
colsharpness (Stage1/rgsbadpix)	no	real	8	$real \ge 0$
Hot column finding: sharpness criterion (see rgsbadpix documentation). Requires withfoundhot=true.
reconstruct (Stage1/rgsevents)	no	boolean	true
On true: spatially adjacent events in the telemetered data are combined into a single ``reconstructed'' event. On false: no event reconstruction. Not applicable to HTR mode data.
withdetcoord (Stage1/rgsevents)	no	boolean	false
On true: in addition to chip coordinates and angular coordinates, detector coordinates for each event are added to the EVENTS table. Parameter detcoord selects among the available coordinate systems. On false: detector coordinates are omitted.
detcoord (Stage1/rgsevents)	no	choice	cam	chip $\mid\,$ cam $\mid\,$ sac
Specifies a standard XMM coordinate system for the output detector coordinates. chip: CHIPCOORD with sub-pixel accuracy. cam: CAMCOORD1. sac: SACCOORD. Requires withdetcoord=true.
betabinning (Stage2/rgsangles)	no	choice	binSize	Range $\mid\,$ binSize
Specifies how the dispersion channels are to be defined. Range: interval to be subdivided (parameters betamin and betamax) and number of channels. binSize: midpoint and width of the first channel (parameters betabinref and betabinwidth) and number of channels.
betamin (Stage2/rgsangles)	no	real	$3\times 10^{-2}$
Lower boundary of the first dispersion channel, in radians. Requires betabinning=Range.
betamax (Stage2/rgsangles)	no	real	$8\times 10^{-2}$
Upper boundary of the last dispersion channel, in radians. Requires betabinning=Range.
betabinref (Stage2/rgsangles)	no	real	$3.578524\times 10^{-2}$
Midpoint of the first dispersion channel, in radians. Requires betabinning=binSize.
betabinwidth (Stage2/rgsangles)	no	real	$1.208\times 10^{-5}$	$real \ge 0$
Dispersion channel width in radians. Requires betabinning=binSize.
nbetabins (Stage2/rgsangles)	no	integer	3400	$integer \ge 1$
Number of dispersion channels.
lambdabinref	no	r	4.005
midpoint of bin for which LAMBDACHA is one [Angstrom]
lambdabinwidth	no	r	0.010
width of lambda bin [Angstroms]
nlambdabins	no	i	3600	$>0$
number of lambda bins.
xdispbinning (Stage2/rgsangles)	no	choice	binSize	Range $\mid\,$ binSize
Specifies how the cross-dispersion channels are to be defined. Range: interval to be subdivided (parameters xdispmin and xdispmax) and number of channels. binSize: midpoint and width of the first channel (parameters xdispbinref and xdispbinwidth) and number of channels.
xdispmin (Stage2/rgsangles)	no	real	$-1\times 10^{-3}$
Lower boundary of the first cross-dispersion channel, in radians. Requires xdispbinning=Range.
xdispmax (Stage2/rgsangles)	no	real	$1\times 10^{-3}$
Upper boundary of the last cross-dispersion channel, in radians. Requires xdispbinning=Range.
xdispbinref (Stage2/rgsangles)	no	real	$-9.126\times 10^{-4}$
Midpoint of the first cross-dispersion channel, in radians. Requires xdispbinning=binSize.
xdispbinwidth (Stage2/rgsangles)	no	real	$1.08\times 10^{-5}$	$real \ge 0$
Cross-Dispersion channel width in radians. Requires xdispbinning=binSize.
nxdispbins (Stage2/rgsangles)	no	integer	170	$integer \ge 1$
Number of cross-dispersion channels.
withpointingcolumn (Stage2/rgsangles)	no	boolean	false
On true: the spacecraft attitude (pointing of the instrument) for each event is added to the EVENTS table. On false: the attitude is omitted.
withmlambdacolumn (Stage2/rgsangles)	no	boolean	false
On true: the primary source $m\lambda$ for each event is added to the EVENTS table. On false: the $m\lambda$ is omitted.
withheliocentriccorr	no	b	Yes
Corrects $m*\lambda$ column from heliocentric velocity
withsunanglecorr	no	b	Yes
Corrects $m*\lambda$ column from Sun angle correction
auxgtitables (Stage3/rgsfilter)	no	list of tables
List of OGIP compliant auxiliary GTI tables for filtering the event list in conjunction with its internal STDGTI0n tables.
withcombmap (Stage3/rgsfilter)	no	boolean	true
rgsfilter produces a filtered exposure map separately for each node, as required by various tasks in the following stages, but a combined map is more convenient to look at and has various uses. On true: the combined exposure map is written to an output dataset. On false: no combined exposure map.
driftbinsize (Stage3/rgsfilter)	no	real	1
Size in arcseconds of the square bins used to group frames according to their aspect drift in dispersion and cross-dispersion. Grouping improves the speed of constructing the exposure maps, at a slight cost in accuracy.
rejflags (Stage3/rgsfilter)	no	list of choices	BAD_SHAPE ON_NODE_INTERFACE ON_BADPIX NEXT_TO_BADPIX ON_WINDOW_BORDER BELOW_ACCEPTANCE	BAD_SHAPE $\mid\,$ ON_NODE_INTERFACE $\mid\,$ ON_BADPIX $\mid\,$ NEXT_TO_BADPIX $\mid\,$ ON_WINDOW_BORDER $\mid\,$ BELOW_ACCEPTANCE
List of rejection flags for filtering the event list.
spatialres (Stage4/rgsregions)	no	integer	5	$integer \ge 2$
Dispersion-axis spacing of vertices for image regions and the background region, specified as the number of vertices across a node. Not applicable to HTR mode data.
orderres (Stage4/rgsregions)	no	integer	3	$integer \ge 2$
Dispersion-axis spacing of vertices for order regions, specified as the number of vertices across a node.
xpsfincl (Stage4/rgsregions)	no	real	90	$0 \le real \le 100$
Size of image regions, specified by the percentage of the cross-dispersion PSF covered between each pair of vertices with the same dispersion coordinate. Not applicable to HTR mode data.
xpsfexcl (Stage4/rgsregions)	no	real	95	$0 \le real \le 100$
Size of the exclusion regions in the background region, specified by the percentage of the cross-dispersion PSF covered between each pair of vertices with the same dispersion coordinate and associated source. Not applicable to HTR mode data.
pdistincl (Stage4/rgsregions)	no	real	90	$0 \le real \le 100$
Size of order regions, specified by the percentage of the pulse-height distribution covered between each pair of vertices with the same dispersion coordinate.
procsrcsexpr (Stage4/rgsregions)	no	string	INDEX==#PRIMESRC
Selection expression indicating which sources to process for image and order regions. The default specifies the primary source only. When restarting rgsproc on its own output, leave this parameter blank to accept the selections already in place.
exclsrcsexpr (Stage4/rgsregions)	no	string	INDEX==#PRIMESRC
Selection expression indicating which sources to exclude from the background region. The default specifies the primary source only. When restarting rgsproc on its own output, leave this parameter blank to accept the selections already in place. Not applicable to HTR mode data.
bkgcorrect (Stage4/rgsspectrum)	no	boolean	no
On true: background-correction is applied to all source spectra. On false: no background correction.
withbkgset (Stage4/rgsspectrum)	no	boolean	true
On true: a background spectrum is produced for each source spectrum. On false: no background spectra.
rebin (Stage4/rgsspectrum)	no	integer	1	$integer \ge 1$
Channel rebinning factor. The events and exposure are rebinned going into the histogram, which gives a more stable result than if the full-resolution spectrum is rebinned later (a very minor point).
withfracexp (Stage4/rgsspectrum)	no	boolean	no
Enables addition of the non-standard (but harmless) FRAC_EXP column to the output spectra. This is the fraction of full exposure in each channel.
withbackgroundmodel (Stage4/rgsspectrum)	no	boolean	no
On true: a background template model spectrum is produced. See rgsbkgmodel for details. On false: no background template model is produced.
exposed (Stage4/rgsspectrum)	no	real	0.1	0-1
Channels with less than this fraction of full exposure are marked as bad in the output QUALITY column.
edgechannels (Stage4/rgsspectrum)	no	integer	2	$integer \ge 0$
The number of channels at the edges of each chip to be marked as bad in the output QUALITY column. For reasons not well understood at this time, the two channels at either edge of every chip do not seem to be properly calibrated.
badquality (Stage4/rgsspectrum)	no	integer	1	0-5
The QUALITY column value used to indicate a bad channel. The default causes bad channels to be discarded automatically by XSPEC. Advanced users of XSPEC may prefer to change this for diagnostic purposes.
withheliocorr (Stage4/rgsspectrum)	no	boolean	no
On true: heliocentriccorr task is executed, writing the VHELICOR keyword in the spectrum header.
witharffile (Stage5/rgsrmfgen)	no	boolean	no
On true: rgsrmfgen will create two independent ARF and RMF files.
rmfbins (Stage5/rgsrmfgen)	no	integer	4000	$integer \ge 1$
Number of rows (incident-energy bins) in the response matrices: effectively the energy resolution. The columns match the channel space of the spectra. The default is fine for general purposes, but very slow to compute; 250 is adequate when only fluxing is intended.
fftdim (Stage5/rgsrmfgen)	no	integer	3	$1 \le integer \le 5$
The wings of the various distributions that are convolved together to form the narrow features of the line-spread function are truncated to limit the size of the convolution space. An increment of one in this parameter doubles the size of the convolution space; the larger the convolution space, the slower the computation and the less power is lost to the truncation. The default is fine for general purposes, but 1 is adequate when only fluxing is intended.
withmirrorpsf (Stage5/rgsrmfgen)	no	boolean	yes
On true: the standard mirror PSF distribution from the CAL is included in the LSF. On false: the mirror PSF is not included. The option to disable the standard mirror PSF is provided primarily for use with extended sources and a custom angular distribution that implicitly contains the mirror PSF.
withdynefferea (Stage5/rgsrmfgen)	no	boolean	yes
On true: execute rgsrmfgen using the dynamic effective area correction based on Chebyshev parameters.
withrectification	no	boolean	no
Use empirical RGS effective area correction
withangdist (Stage5/rgsrmfgen)	no	boolean	no
On true: the user-defined angular distribution is included in the LSF. On false: it is not included. This option is provided for the purposes of extended-source analysis, but the imaginative user may find other applications for it.
angdistset (Stage5/rgsrmfgen)	no	file	angdist.txt
An ASCII formatted distribution in RGS dispersion offset angle, for use in generating a customized LSF, presumably for an extended source. See rgsrmfgen for details on the file format. Requires withangdist=true.
mergeorders (Stage5/rgsfluxer)	no	boolean	false
On true: all the spectra (both instruments, all exposures and reflection orders) are combined together in a single fluxed spectrum. On false: a separate fluxed spectrum is produced for each reflection order.
flxformat (Stage5/rgsfluxer)	no	choice	dal	dal $\mid\,$ ascii $\mid\,$ qdp
Specifies the format of the output fluxed spectrum. dal: FITS-encoded SAS dataset. ascii: basic ASCII-encoded text file. qdp: text file formatted as input to qdp.
flxmode (Stage5/rgsfluxer)	no	choice	wavelength	wavelength $\mid\,$ energy
Specifies the units for defining the output fluxing bins (parameters flxmin and flxmax). wavelength: units of Å. energy: units of keV.
flxmin (Stage5/rgsfluxer)	no	real	4	$real \ge 0$
Lower edge of the first output bin in the units set by flxmode. The default is not appropriate for flxmode=energy.
flxmax (Stage5/rgsfluxer)	no	real	39	$real \ge 0$
Upper edge of the last output bin in the units set by flxmode. The default is not appropriate for flxmode=energy.
flxbins (Stage5/rgsfluxer)	no	integer	3400	$integer \ge 1$
Number of output bins.
flxquality (Stage5/rgsfluxer)	no	list of integers		$0 \le integer \le 5$
This parameter controls how the quality flags from the input spectrum files are propagated into the output fluxed spectrum. If the quality flag of an input spectral channel is not represented in this list, the associated count rate is simply discarded. Where multiple channels, either from the same or from different spectra, overlap the same output bin, the output quality is degraded to the worst input quality. This ranking is set by the order of the list itself: from highest quality to lowest. Thus the list ``0 2 1'' preserves all input channels and degrades the quality in the sequence, ``good'' to ``dubious'' to ``bad''. The default preserves only the ``good'' channels. When only one quality value is permitted, the quality column is omitted from the output file. Quality flags three, four and five are defined within XSPEC, but are not currently used by rgsspectrum.
withflxnan (Stage5/rgsfluxer)	no	boolean	false
Undefined flux values naturally occur at spectral channels where there is no exposure, such as in the gaps between chips, and are represented by NaN (IEEE standard encoding). Sadly, many standard analysis packages do not react well to this. On true: all instances of NaN in the output are replaced with the specified finite alternative (parameter flxnan). On false: NaN is permitted in the output.
flxnan (Stage5/rgsfluxer)	no	real
Value used instead of NaN (or ``no'', in the case of flxformat=qdp) to indicate an undefined value in the output fluxed spectrum. Requires withflxnan=true.
timebinsize	no	1000	real	$>0$
Size of time bins.
withbkgsubtraction	no	bool	no
Enable background subtraction
Parameter	Mand	Type	Default	Constraints