Changes between Version 8 and Version 9 of Background_Dark_Model
- Timestamp:
- Mar 8, 2012, 1:26:12 PM (14 years ago)
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Background_Dark_Model
v8 v9 71 71 Based on this observation, I'm currently constructing a new dark master from data taken after 2011-05-01, which should fit all exposures after this point. However, there is no clear idea why this mode has become dominant. A voltage change was done around this time to solve the STS Astrometry bug, but OTA67 was not one of those with a change. 72 72 73 [[Image 74 [[Image 73 74 == March 8, 2012 == 75 76 The new dark has finished, and although there does seem to be a weak trend in the residual slopes with dateobs, these slopes have been greatly decreased relative to the previous dark iteration: 77 78 [[Image(dateobs_new_dark.png)]] 79
