Grouping Normal Type Ia Supernovae by UV to Optical Color Differences release_ms3tdd7qv5hyjjssqd4lhoajwu

by Peter A.Milne, Peter J. Brown, Peter W. A. Roming, Filomena Bufano, Neil Gehrels

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abstracts[] {'sha1': '7cf73db9260ab2e888c35f4196976d8c803926c1', 'content': 'Observations of many SNe Ia with the UVOT instrument on the Swift satellite\nhas revealed that there exists order to the differences in the UV-OPT colors of\nnormal SNe. We examine UV-OPT color curves for 25 SNe Ia, dividing them into 4\ngroups, finding that ~1/3 of these SNe Ia have bluer UV-OPT colors than the\nlarger group, with these "NUV-blue" SNe Ia 0.4 mag bluer than the "NUV-red" SNe\nIa in u-v. Another group of events feature colors similar to NUV-red SNe Ia in\nthe u-v to uvw1-v colors, but similar to the NUV-blue SNe Ia in the uvm2-v\ncolor. We name these events "MUV-blue". The last group initially has colors\nsimilar to NUV-red SNe Ia, but with color curves that feature more modest\nchanges than the larger NUV-red group. These "irregular" events are comprised\nof all the NUV-red events with the broadest optical peaks, which leads us to\nconsider this minor group a subset of the NUV-red group. When so separated and\nthe accounting is made for the rapid time evolution of the UV-OPT colors, we\nfind that the scatter in two NUV-OPT colors, u-v & uvw1-v, is at the level of\nthe scatter in b-v. This finding is promising for extending the cosmological\nutilization of SNe Ia into the NUV. We generate spectrophotometry of SNe Ia\nthat have been observed with HST and argue that there is a fundamental spectral\ndifference in the 2900-3500A wavelength range, a range suggested to be\ndominated by absorption from iron-peak elements. The NUV-blue SNe Ia feature\nless NUV absorption than the NUV-red SNe Ia. We show that all the NUV-blue SNe\nIa in this sample have also featured evidence of unburned carbon in optical\nspectra, whereas only one NUV-red SN Ia features that absorption line. Every\nNUV-blue event also exhibits a low gradient of the SiII 6355A absorption\nfeature, but many NUV-red events also exhibit a low gradient, perhaps\nsuggestive that NUV-blue events are a subset of the larger LVG group.', 'mimetype': 'text/plain', 'lang': 'en'}
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{'index': 1, 'creator_id': None, 'creator': None, 'raw_name': 'Peter J. Brown', 'given_name': None, 'surname': None, 'role': 'author', 'raw_affiliation': None, 'extra': None}
{'index': 2, 'creator_id': None, 'creator': None, 'raw_name': 'Peter W. A. Roming', 'given_name': None, 'surname': None, 'role': 'author', 'raw_affiliation': None, 'extra': None}
{'index': 3, 'creator_id': None, 'creator': None, 'raw_name': 'Filomena Bufano,\n Neil Gehrels', 'given_name': None, 'surname': None, 'role': 'author', 'raw_affiliation': None, 'extra': None}
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license_slug ARXIV-1.0
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release_date 2013-08-12
release_stage submitted
release_type article
release_year 2013
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title Grouping Normal Type Ia Supernovae by UV to Optical Color Differences
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arxiv.base_id 1308.2703
arxiv.categories ['astro-ph.CO']
arxiv.comments Accepted to the Astrophysical Journal Updated version: Sept 16, 2013
superceded True