Unschedulable Visit FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser Visit 2 added for F814W filter, and the abstract was updated to reflect this change. -1010398682 ----- Attempting Submission 1 (Mon Jul 25 16:42:04 GMT 2022) ----- HST Phase II Proposal 17014 successfully submitted. Receipt: # 17014-1 ----- Attempting Submission 2 (Mon Jul 25 19:11:02 GMT 2022) ----- HST Phase II Proposal 17014 successfully submitted. Receipt: # 17014-2 ----- Attempting Submission 3 (Mon Jul 25 19:50:21 GMT 2022) ----- ----- Attempting Submission 4 (Tue Mar 21 18:42:48 GMT 2023) ----- ----- Attempting Submission 5 (Thu Mar 23 13:05:10 GMT 2023) ----- This is a Cal/WFC3 proposal. Abstract was updated to say that Visit 2 has been added for the F814W filter. WFC3 UVIS Shutter Monitoring We monitor the WFC3 UVIS shutter performance. The exposures in F555W need to be identical to previous cycles. Images with exposure times ranging from 0.5 to 17 seconds will be used to compare the photometric behavior of each shutter blade, for short vs long exposures and check for shutter shading effects. The first exposure of 0.5sec cannot be used since the lamp would be still heating during this exposure, so we will take a set of three 0.5sec exposures. Internal flats in each of the 4 amps will be used to monitor the repeatability and shutter shading effects. We want to iclude some wavelength dependence, so this proposal now includes exposures in F814W filter, exposure times for which have been estimated using information from WFC3 ISR 2008-21. WFC3/Cal proposal. WFC3 Team Member 0 false false RESTRICTED The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. 1664827589000 180.0 (Tic-Visit :proposal-id 17014 :visit-id "01" :proposal-version -1 :trans-version "20220516" :date "25-Jul-2022 12:39:47.0" :trans-errors '(:WARNINGS 2 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 0.0 :data-volume 2021216 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17014 :visit-id "01" :obset-id "01" :pcs-mode "GYRO" ) (Tic-Orbit :proposal-id 17014 :visit-id "01" :orbit-number 1 :pcs-time 0 :si-vis-utilization 0 :al-overhead-at-end 0 :internal-dur-at-end 3348 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 This assumes Tungsten lamp 3. (2800 e-/sec/pix through F555W in TV3 testing) This assumes Tungsten lamp 3. (2800 e-/sec/pix through F555W in TV3 testing) This assumes Tungsten lamp 3. (2800 e-/sec/pix through F555W in TV3 testing) (Tic-Visit :proposal-id 17014 :visit-id "02" :proposal-version -1 :trans-version "20220630" :date "21-Mar-2023 14:37:22.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 0.0 :data-volume 2021216 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17014 :visit-id "02" :obset-id "02" :pcs-mode "GYRO" ) (Tic-Orbit :proposal-id 17014 :visit-id "02" :orbit-number 1 :pcs-time 0 :si-vis-utilization 0 :al-overhead-at-end 0 :internal-dur-at-end 3318 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 This assumes Tungsten lamp 3. (20,000 e-/sec/pix through F814W, WFC3 ISR 2008-21) This assumes Tungsten lamp 3. (20,000 e-/sec/pix through F814W, WFC3 ISR 2008-21)