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Method
The program uses a detector matrix file, default XRTCAL:DRMPSPC,
to calculate the basic response. To convert this response into an
effective area the response from the matrix is multiplied by the
energy dependent correction array written into the datafile by
XRTCORR. The corrections program should have written an array
MORE.ASTERIX.INSTRUMENT.ENCORR(n).DATA_ARRAY into the datafile. If
this isn't found then the program will exit with a message to that
effect.
Next: Scope Up: XRTRESP Prev: Radial spectra