MERGING RULE VIOLATED DURING AUTOMATIC MERGING
MERGING RULE VIOLATED DURING AUTOMATIC MERGING
MERGING RULE VIOLATED DURING AUTOMATIC MERGING
MERGING RULE VIOLATED DURING AUTOMATIC MERGING
MERGING RULE VIOLATED DURING AUTOMATIC MERGING
MERGING RULE VIOLATED DURING AUTOMATIC MERGINGResubmitted after swapping cutting the F814W exposures of visit 03, i.e. P330E.-452397674----- Attempting Submission 1 (Tue Jun 28 20:05:51 GMT 2022) -----
----- Attempting Submission 2 (Fri Aug 19 16:24:42 GMT 2022) -----
----- Attempting Submission 3 (Thu Oct 06 17:25:21 GMT 2022) -----
----- Attempting Submission 4 (Fri Oct 14 20:20:14 GMT 2022) -----
----- Attempting Submission 5 (Thu Nov 10 19:58:20 GMT 2022) -----
----- Attempting Submission 6 (Wed May 31 20:10:14 GMT 2023) -----
Your proposal could not be saved.
Submission aborted.
----- Attempting Submission 7 (Fri Jun 02 13:27:26 GMT 2023) -----Merging rule violationWFC3 UVIS Time Dependent SensitivityThis program acquires scanned observations for monitoring the relative changes in the WFC3/UVIS photometric throughput. The spectrophotometric white dwarf standard stars GD153 and GRW70, and G-type star P330E, are scanned in a subset of filters periodically over the year. Historically, this program was intended as a monitor of the UV filters as they provide a means to detect contaminants on the instrument optics, with one or two visible/red filters serving as a control. Since then, additional filters in the visible and red have been added to the program to expand the monitor to longer wavelengths. The observing cadence is roughly once a month though some exceptions are required to accommodate visibilities.Each visit of the 12 in this program spends one orbit on a single standard star: 5 visits each for the white dwarfs GD153 and GRW70 and 2 visits for the solar-type star P330e. The white dwarf visits are alternated during the cycle, as close to every four weeks as visibilities will allow. The P330E visits are placed in the first and last quarters of the cycle, phased to fall between the white dwarf visits.
Each white dwarf visit possesses a similiar structure: roughly a dozen scans on UVIS1 and about half that number on UVIS2, in a variety of filters. As P330e is a solar type star, UV exposure times are significantly longer than for the white dwarfs and as a consequence, fewer exposures fit into the orbit. When possible, scans use the same parameters: 60s exposure time, 7.5'' scan at 0.125''/s. The longer exposures (P330e in UV) require several hundred seconds at 0.01''/s, for scans of 3-5" in length. To maximize "time-on-target", scans alternate between 'reverse' and 'forward' direction in each visit.0falsefalseRESTRICTEDCALIBRATIONPHOTOMETRICThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000STARDAThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000CALIBRATIONPHOTOMETRICNOThis object was generated by the targetselector and retrieved from the SIMBAD database.GSC-02581-02323J2000The scheduling data was generated by CASM 30.3.CASM was run in Phase II mode.Visit 1 of 5 for GRW70.(Tic-Visit
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(Tic-Orbit
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:si-vis-utilization 2884
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)true10The scheduling data was generated by CASM 30.3.CASM was run in Phase II mode.Visit 1 of 2 P330E.1677197664000295.3622824610829(Tic-Visit
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)true10The scheduling data was generated by CASM 30.3.CASM was run in Phase II mode.Visit 2 of 5 for GRW70.1677552443000205.30346896124502(Tic-Visit
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)true10The scheduling data was generated by CASM 30.3.CASM was run in Phase II mode.Visit 2 of 5 for GD153.1683988909000140.0027899416164(Tic-Visit
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)true10The scheduling data was generated by CASM 30.3.CASM was run in Phase II mode.Visit 3 of 5 for GRW70.1685009942000145.70971022714838(Tic-Visit
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)true10The scheduling data was generated by CASM 31.0.CASM was run in Phase II mode.Visit 2 of 3 P330E.1687093957000180.2(Tic-Visit
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)true10The scheduling data was generated by CASM 30.3.CASM was run in Phase II mode.Visit 5 of 5 F218W,(Tic-Visit
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)true10The scheduling data was generated by CASM 30.3.CASM was run in Phase II mode.Visit 3 of 3 P330E.(Tic-Visit
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)true10The scheduling data was generated by CASM 30.3.CASM was run in Phase II mode.Visit 5 of 5 for GD153.(Tic-Visit
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