Changes between Version 7 and Version 8 of NightOperations/Commissioning/Plans/20160528
- Timestamp:
- May 27, 2016 9:57:15 PM (8 years ago)
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NightOperations/Commissioning/Plans/20160528
v7 v8 136 136 137 137 138 === Test EGS setup === 139 140 See e-mail from Steve Finklestein. Unpack that information and see if you can use it to setup on one of the EGS fields. Compare setup to Gstar results. 141 142 138 143 ------------- 139 144 … … 145 150 We'd also like to add getting a larger number of flat exposures to the long-term operations procedures. This is for monitoring small changes in the pixel-to-pixel response for VIRUS over time. The cadence would be about once a week, and after any unit has been pumped and recooled, and we want LDLS 20 flats taking each time for this. 146 151 152 lots of bias datasets for VIRUS - we want to see if there is any correlation between small changes we see in the structure of the bias and CCD temperature or enclosure temperature. Since many of the CCDs are floating in temperature depending on the enclosure temperature, we may be causing very small changes in bias. We'd like to look for this and any other instability that there might be. So if you're closed or have poor conditions, getting say 10 bias sets distributed through the night and recording the CCD, and enclosure temps for each would be a useful dataset. 153