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Assigned ID: 323
----- Attempting Submission 1 (Fri Apr 08 00:15:09 GMT 2016) -----
HST Phase I Proposal 323 (historic_sne_c24.apt) successfully submitted.
Receipt: # 323-1
----- Attempting Submission 2 (Fri Apr 08 21:26:20 GMT 2016) -----
Changed exposure sequences to make exposure times more even, and checked that FLASH is only used for F438W UVIS exposures.
1475920824
----- Attempting Submission 1 (Wed Jul 20 23:38:14 GMT 2016) -----
----- Attempting Submission 2 (Thu Jul 21 18:40:13 GMT 2016) -----
----- Attempting Submission 3 (Fri Jul 22 22:03:55 GMT 2016) -----
HST Phase II Proposal 14786 (historic_sne_c24_updated.apt) successfully submitted.
Receipt: # 14786-3
----- Attempting Submission 4 (Fri Jul 22 22:10:00 GMT 2016) -----
----- Attempting Submission 5 (Fri Sep 02 21:44:36 GMT 2016) -----
HST Phase II Proposal 14786 (14786.apt) successfully submitted.
Receipt: # 14786-5
----- Attempting Submission 6 (Wed Sep 07 19:30:25 GMT 2016) -----
Progenitor Masses for Every Nearby Historic Core-Collapse Supernova
Some of the most energetic explosions in the Universe are the core-collapse supernovae (CCSNe) that arise from the death of massive stars. They herald the birth of neutron stars and black holes, are prodigious emitters of neutrinos and gravitational waves, influence galactic hydrodynamics, trigger further star formation, and are a major site for nucleosynthesis, yet even the most basic elements of CCSN theory are poorly constrained by observations. Specifically, there are too few observations to constrain the progenitor mass distribution and fewer observations still to constrain the mapping between progenitor mass and explosion type (e.g. IIP IIL, IIb, Ib/c, etc.). Combining previous measurements with 9 proposed HST pointings covering 13 historic CCSNe, we plan to obtain progenitor mass measurements for all cataloged historic CCSNe within 8 Mpc, optimizing observational mass constraints for CCSN theory.
This program will observe 9 pointings covering 13 SNe locations. The NGC6946 pointings cover 2 SNe per pointing, and the SN2002AP will be in the parallel pointing for SN2003GD. All other pointings cover one SNe each. Each observation has 4 exposures in each camera per orbit, with a dither pattern designed to get approximately 0.5 pixel sampling in both cameras.
Stellar Physics
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