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ulammers |
1.1 |
ChangeLog for emos-aduconv |
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dlumb |
1.5 |
VERSION 0.5 - 2000-06-23 (DL) |
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The initial flight calibration revealed discrepancies at the O edge |
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and the lowest energy reponses. These were attributed mainly to |
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systematic errors in the monitoring process at the Orsay synchrotron. |
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New empirical fits to the data were provided by Leicester, and these |
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have been compared with new SCISIM runs, utilising the best latest |
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electrode structure used in the Leicester analystical QE model fit. A |
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combination of LUX data, and an extension BELOW the Si L edge for the |
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SCISIM data allows a hopefully better fit. In addition I have modified |
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the QE's for the outer CCDs of each camera, where there are systematic |
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differences in QE at > 5keV. These can be attributed to ddifferences |
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in silicon resistivity translating to different depletion depths. The |
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QE data for this at Orsay is equivocal, so I take average trends in |
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increased efficiency between 5 and 12keV and allocate a best estimate |
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of increased depletion depth to this, and in return modify the overall |
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QE curves as a result. I am suspicious, though that all QE's are |
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GREATER tahn the central CCD, and this may indicate a systematic bias |
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in the measurment method at Orsay. |
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The new data sets should give good results to about 10% accuracy at |
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worst case small energy scales (eg EXAFS scales at silicon edges etc.) |
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dlumb |
1.4 |
VERSION 0.4 - 2000-05-23 (DL) |
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FIxed error of missing pattern 1 data for CCD5 |
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dlumb |
1.3 |
VERSION 0.3 - 2000-02-23 (DL) |
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FIxed numerical problem in the data files (some values >>1 ) |
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ulammers |
1.2 |
Version 0.2 - 2000-02-17 (UL) |
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+ fixed minor problem with REGION expression in data files |
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ulammers |
1.1 |
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ulammers |
1.2 |
Version 0.1 - 2000-02-09 (DL) |
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ulammers |
1.1 |
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+ created by DL |