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C(I): The Observed Spectrum

To obtain the observed spectrum (C(I)), for a given observation, XSPEC uses two files: the data file, and the background file (for FITS file format see Arnaud, George & Tennant 1992gif). The data file tells XSPEC how many total photon counts were detected by the instrument in a given channel. XSPEC then uses the background file to derive a background-subtracted C(I) in units of counts per second. The background is scaled to the data by the ratio of the BACKSCAL keywords in the data and background files. It also is scaled for exposure times (EXPOSURE keyword). The background-subtracted count rate is given by :

displaymath10261

where D(I) and B(I) are the counts in the data and background files; tex2html_wrap_inline10267 and tex2html_wrap_inline10269 are the exposure times in the data and background files; and tex2html_wrap_inline10271 and tex2html_wrap_inline10273 are the BACKSCAL values from the data and background files.

When this is done XSPEC has an observed spectrum to which the model spectrum can be fit.



Keith Arnaud (kaa@genji.gsfc.nasa.gov)
Wed May 28 10:59:33 EDT 1997