Документ взят из кэша поисковой машины. Адрес оригинального документа : http://xmm.vilspa.esa.es/sas/6.5.0/doc/rgssuperrmf/node4.html
Дата изменения: Tue Aug 16 07:54:46 2005
Дата индексирования: Sat Dec 22 12:12:48 2007
Кодировка:
Поисковые слова: п п п п п п п п п п п п п п п р п р п р п р п

XMM-Newton Science Analysis System


rgssuperrmf (rgssuperrmf-1.0.4) [xmmsas_20050815_1803-6.5.0]

Meta Index / Home Page

Parameters

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

Parameter	Mand	Type	Default	Constraints
phalist	yes	typelist of files
A list of spectrum files from a set of observations, referring to one RGS instrument and one spectral order. These spectra files must be produced using the attstyle=user and associated parameters from a call to rgsproc.
evlist	yes	typelist of files
A list of accompanying event list files, in the same order as the spectra files. Note, the file names are not derived from the spectra files.
srclist	yes	typelist of files
A list of accompanying source list files, in the same order as the spectra files
bkglist	yes	list of files
A list of background spectrum files from a set of observations observations
withspeccombine	no	boolean		yes
If this parameter is set to yes, the spectra files of the input lists will be combined to produced a combined spectrum file each for both spectra and background spectra files.
filermf	no	file		resultantmatrix.ds
Filename for final response matrix
filepha	no	file		combinedspectra.ds
Filename for final spectrum
filebkg	no	file		combinedback.ds
Filename for final background spectrum
The remaining parameters are exactly the same as those for the task rgsrmfgen, and are used when calling this task within rgssuperresponse, with the exception that spectra files are compulsory for this task and therefore the option that appears in rgsrmfgen, withspectrum, has been removed and is always true.
emax	no	real	2.8	non-negative
When creating a new response matrix, this is the upper edge of the highest incident-energy bin to be included.
emin	no	real	0.3	non-negative
When creating a new response matrix, this is the lower edge of the lowest incident-energy bin to be included. When overwriting part of an existing matrix (newrmf=no), this identifies the lower incident-energy bin in the interval to be recomputed. This value will be lowered automatically as necessary to maintain the contiguity of the bins, and can be used to extend the range of the existing matrix.
rows	no	integer	4000	positive
The number of incident-energy bins to cover the range from emin to emax.
phachannels	no	integer	3400	positive
The number of pha channels.
withmirrorpsf	no	boolean	yes
Whether to convolve the standard mirror PSF distribution into the LSF. This option should be used with care and knowledge. An appropriate circumstance for omitting the mirror PSF is when a custom angular distribution is provided (withangdist=yes) that empirically establishes the PSF contribution.
withangdist	no	boolean	no
Whether to convolve a custom angular distribution into the LSF. This option should be used with care and knowledge. Enables parameter angdistset. Note that this distribution is one-dimensional, an arbitrary function of dispersion off-axis angle. It is rebinned onto the dispersion channel space according to the order and central incident energy of each LSF. The problem of reducing a two-dimensional image to this one-dimensional distribution is left to the user.
angdistset	no	file	angdist.txt
An ASCII file containing a one-dimensional angular distribution along the axis of dispersion in arc minutes. Not modified. Each line of the file describes a distribution bin in terms of the start and stop angles, and the value assigned to that bin. The distribution may be normalized to any value, though unity is expected and recommended. See the input files descriptions for further details.
Parameter	Mand	Type	Default	Constraints