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In order to check that absorption, emission and reemission spectra and timing distributions are used correctly, a number of root histograms can be created. These are implemented via a flag in the SCBU
bank and the symbolic command
$scint_debug_hist $on
. The histograms are initiated in the routine INPHI and a message is written to standard output, detailing what each histogram shows.
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2009-09-09