THE XMM-NEWTON ABC GUIDE, STREAMLINED
Fit an EPIC Spectrum with Xspec (Locally Installed)
We will do some simple spectral fitting, using as an example the source and background that was extracted from the Lockman Hole observation (Obs ID 0123700101) and its RMF and ARF files. All tasks will be called from the command line.
For this example, we are interested in just a quick fit to see what we are dealing with, so we will rebin the data. The procedure grppha from FTOOL provides an excellent mechanism to do that. The following commands not only group the source spectrum for Xspec but also associate the appropriate background and response files for the source. This is done simply by calling the task and editting parameters as is appropriate:
>ftools >grppha Please enter PHA filename mos1_pi.fits ! input spectrum file name Please enter output filename mos1_pi_grp30.fits ! output grouped spectrum GRPPHA chkey BACKFILE bkg_pi.fits ! include the background spectrum GRPPHA chkey RESPFILE mos1_rmf.fits ! include the RMF GRPPHA chkey ANCRFILE mos1_arf.fits ! include the ARF GRPPHA group min 30 ! group the data by 30 counts/bin GRPPHA exitNext, use Xspec to fit the spectrum, editting the parameters as needed.
>xspec XSPEC> data mos1_pi_grp30.fits ! input data XSPEC> ignore 0.0-0.2,6.6-** ! set a range appropriate for the data, in keV XSPEC> model pow ! set spectral model to a power law 1:powerlaw:PhoIndex> 2.0 ! set the power law index to 2.0 2:powerlaw:norm> ! default model normalization XSPEC> renorm ! renormalize the model spectrum XSPEC> fit ! fit the model to the data XSPEC> setplot device /xw ! set the plot device XSPEC> setplot energy ! plot energy along the X axis XSPEC> plot ldata ratio ! plot two panels with the log of the data and ! the data/model ratio values along the Y axes XSPEC> exit ! exit Xspec Do you really want to exit? (y) yThe spectrum is shown in Figure 1.
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