The list of Investigators does not match the STScI records for this program. MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU I have tried to schedule the visits so that they will all occur within 5 days of the first visit, and within the same intra-anneal period. I looked at the current anneal program (CAL-16967, PI=Baggett) and scheduled these visits to occur between the windows. I tried to keep these visits within the 1800s window, but it doesn't seem to want to readout the first exposure during the second, so the readout extends beyond 1800s. Hope that's not a problem. I know that the standard darks do two 900s images in an internal orbit and take many hundreds of internal orbits per year that way, but since I have 15 visits here that need to be executed within ~5 days, I wanted to give you all scheduling flexibility. 759425116 ----- Attempting Submission 1 (Mon Oct 31 18:21:13 GMT 2022) ----- It's referrin to the over-run on the internal visit. If I could make it dump the buffer from the first exposure in the visit during the second exposure, rather than waiting until they're both done, then it would fit. Hopefully this won't be a problem. WFC3 UVIS CTE Internal Monitor The goal of his program is to demonstrate a new way to pin the pixel-based CTE model. We will take a set of ~500s dark exposures with a variety of post-flash levels, from 0e to 30,000e (the maximum possible). Each expousure by design should have the same WPs (warm pixels) before readout, but the various backgrounds will result in different CTE losses for each WP in each exposure. By studying the survival of the electrons in each WP, we can compare the pixel-based model's predictions for losses-vs-WP intensity-vs-background against the results seen in the actual detector. Previous programs have taken sets of short darks and long darks, but there were not always enough WPs in the short darks to make those exposures useful. This was particularly the case at higher background levels where fainter WPs cannot be reliably measured on account of the noise in the background itself. The longer darks employed for all exposure levels here should alleviate these concerns. The current plan is to take a program like this in our routine yearly cal suite. We take a uniform set of darks with a range of post-flash levels. The goal is to have each dark exposure be ~500s. In practice, the actual achieved darktime will probably be ~503s on account of overheads, but the important things is that the time be the same for all exposures. This program involves 15 internal orbits. In each orbit we can take two 500s darks with different background levels via postflash within the 1800s range (readout extends longer). The levels we will probe are: 0e, 1e, 2e, 4e, 7e, 10e, 15e, 20e, 25e, 30e, 40e, 50e, 65e, 80e, 100e, 120e, 150e, 200e, 300e, 500e, 750e, 1000e, 1500e, 2500e, 4000e, 7500e, 10000e, 15000e, 20000e, and, 30000e. The first 22 PF levels can be explored with the standard FLASH requirement, which imparts about 2.5e per second of post-flash, up to a maximum background of 1000e. The remaining 8 PF levels have to be explored with MED current, which imparts 75e per second and can achieve a background of 30,000. 0 false false RESTRICTED /private/var/folders/_d/p5sz3s3n6tsf5mjyrwch42zc000496/T/OPVisit16574734916401241443.xml Timing link suitability includes constraints ([02 After 01 by at most 5.0 days] [03 After 01 by at most 5.0 days] [04 After 01 by at most 5.0 days] [05 After 01 by at most 5.0 days] [06 After 01 by at most 5.0 days] [07 After 01 by at most 5.0 days] [08 After 01 by at most 5.0 days] [09 After 01 by at most 5.0 days] [10 After 01 by at most 5.0 days] [11 After 01 by at most 5.0 days] [12 After 01 by at most 5.0 days] [13 After 01 by at most 5.0 days] [14 After 01 by at most 5.0 days] [15 After 01 by at most 5.0 days]) The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. 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