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DatePhoton SourceCarrier ID 0/1Digital Card ID 0/1Analog Card ID 0/1Experiment/RunGain FileComment
2016-04-14Cu K-alpha (8 keV)996663297/37916508261232098304/9532062832655595777/520093719xcs01116/95gainPixelCorr_passZero_r95_c1.txtFrom Philip Hart
2016-06-30Cu K-alpha

996477441/2264924170

1794137088/403490827

2397900801/4076863512

xcs06016/37gainPixelCorr_passZero_r37_c1.txtFrom Philip Hart
2016-06-30Cu K-alpha

996579585/553648138

1232098304/1221641739

2650251521/3976200215

xcs06016/37gainPixelCorr_passZero_r37_c2.txtFrom Philip Hart
2016-06-30Cu K-alpha

996663297/3791650826

1232098304/953206283

2655595777/520093719

xcs06016/37gainPixelCorr_passZero_r3335_c3.txtFrom Philip Hart
2016-07-01Ni fluorescence998779393/1174405221794137088/4034908272669921025/100663319xcs06016/52gainPixelCorr_passZero_r52_c2.txtFrom Philip Hart
2016-07-01Ni fluorescence996513537/20803747941794135040/9403617392398406657/419430424xcs06016/52gainPixelCorr_passZero_r52_c3.txtFrom Philip Hart
2016-07-01Cu K-alpha996432897/35903242341232100352/11545328752654088449/33554455xcs06016/37gainPixelCorr_passZero_r37_c0.txtFrom Philip Hart
2016-10-21 As above  xcsm9816/2-27,45-49gainPixelCorr_passZeroL_r2049_c2.txtFrom Philip Hart
2017-06-06Cu K-alpha997010433/31708938341794137088/4034908272403244545/1224736792mfx01316/6,7 gain3PixelCorr_passZero_r6007_c0.txtFrom Philip Hart, fit statistics might be marginal so consider using the alternative non-fit results below
  As above    From Philip Hart, uses mode instead of gaussian fit because of marginal statistics

Note that the following script can be used to dump out the EPIX ID numbers:

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