xmmpsf: xmm surface brightness model
Mixing model for XMM data. Mixes the spectra between datagroups based on the
PSF overlap between selected regions. A surface brightness model is required
to calculate the mixing and this can be supplied in several ways. If
XMMPSF-IMAGE has been set to some image file (using xset) then this
image will be used for the surface brightness distribution. If XMMPSF-IMAGE
has not been set then either a beta or two power-law model is used. In this
case the model parameters determine the shape of the surface brightness
distribution. If XMMPSF-RA and XMMPSF-DEC are set they are used as the center
of the distribution. They should be specified either in decimal degrees or
as hh:mm:ss.s and dd:mm:ss.s. If XMMPSF-RA and XMMPSF-DEC are not set then
the centroid of the wmap will be used as the center of the surface
brightness distribution.
The model works by calculating the mixing factors. It will recalculate these
factors if any of the XMMPSF-* or any of the model parameters are changed.
Calculating the mixing factors is very slow so should be avoided as much as
possible. To speed things up, it is possible to save the mixing factor array
to a FITS file and re-use it during a later calculation. To save a mixing
factor calculation, prior to loading the mixing model (using the model
command), use xset to set the variable XMMPSF-MIXFACT-OFILEn to the
name of the output FITS file, and where n is an integer corresponding to the
observation number:
XSPEC12> xset XMMPSF-MIXFACT-OFILE1 fact_obs1.fits
Conversely, a saved factor array can be read in by setting XMMPSF-MIXFACT-IFILEn:
XSPEC12> xset XMMPSF-MIXFACT-IFILE1 fact_obs1.fits
Multiple observations can be fit simultaneously. In this case the observations
should be read in each datagroup in the same order, e.g.
XSPEC12> data 1:1 obs1reg1 1:2 obs2reg1 1:3 obs3reg1 2:4 obs1reg2 2:5 obs2reg2
par1 |
Alpha (not used if Switch=0) |
par2 |
Beta |
par3 |
Core (arcmin) |
par4 |
Switch (0 = beta model, 1 = 2-power-law) |
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Last modified: Friday, 23-Aug-2024 13:20:40 EDT
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