AIDA
GELINA
BRIKEN
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CARME
StellarModelling
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AIDA
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> 10.23 Low energy calibration program now produces relative gain coefficients in a format that can be used with AIDASort > > using sorted alpha data Oct18/R29* > > 30 2.0GB files of data > > LHS: Data sorted without relative gain-matching > > RHS: Data sorted with relative gain-matching > > Attachments (1-4) - DSSD1 - Ey-Ex > > - Ey vs Ex > > - Energy difference vs x strip > > - Energy difference vs y strip > > Attachments (5-8) - DSSD2 - Ey-Ex > > - Ey vs Ex > > - Energy difference vs x strip > > - Energy difference vs y strip > > Attachments (9-12) - DSSD3 - Ey-Ex > > - Ey vs Ex > > - Energy difference vs x strip > > - Energy difference vs y strip > > Attachments (13-16) - DSSD4 - Ey-Ex > > - Ey vs Ex > > - Energy difference vs x strip > > - Energy difference vs y strip > > Attachments (17-20) - DSSD5 - Ey-Ex > > - Ey vs Ex > > - Energy difference vs x strip > > - Energy difference vs y strip > > Attachments (21-24) - DSSD6 - Ey-Ex > > - Ey vs Ex > > - Energy difference vs x strip > > - Energy difference vs y strip > > > Attachment 25 - Table comparing peak centroids and peak width (deviation, sigma) of Ey - Ex plots before and after gainmatching > > - numbers found with simple gaussian fit > > > > > > >
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