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 SUThis is nearly identical to the program submitted last year (CAL-17259).
It is designed to be all taken during the same intra-anneal period. I have
put in three options, but could easily put in more if it is hard to schedule
in the Nov-Dec-Jan-Feb timeframe.654694403----- Attempting Submission 1 (Fri Jul 21 18:38:56 GMT 2023) -----It is a calibration program that does internals. Perhaps that does not require restricted mode.
Feel free to unselect that if I toggled that in error.
The warnings are that the readout portion of the internals go a bit beyond the recommended
lentgth. That seems ok, since this happens with dark programs to an even larger degree. This
program involves only 15 internal orbits, so it shouldn't be too hard to find times when it can
go. I can reduce the darktime if the length of the internal orbits causes problems.WFC3 UVIS CTE Internal MonitorThe goal of this yearly monitor program is to provide a supplemental way to monitor and re-pin the pixel-based CTE model. The program will take a set of ~500s dark exposures with a variety of post-flash levels -- from 0e to 30,000e (the maximum possible). By design, each expousure should have the same WPs (warm pixels) before readout (hence the same darktime). As the detector is read out, though, the various backgrounds will result in different CTE losses for each WP in each exposure. By studying the survival-to-readout 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 explore all issues. 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 in this regular monitor program should alleviate these concerns. Last year, CAL-17259 was the first formal pilot program of this monitor program. This year it has become a regular monitoring program.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 thing is that the effective dark 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. 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. Backgrounds above that would require a PF of longer than 500s, which would increase the darktime above that of of the other exposures. In principle, we could use tungsten lamps to get higher than 30,000 counts but thus far it does not seem critical to have an extra PF level beyond 30,000e.Anderson has studied CTE in ACS/WFC and WFC3/UVIS for over 10 years.
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