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The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am
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Tartaglia_2018_ApJ_853_62.pdf
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Final Published Version
Author
Tartaglia, L.Sand, David J.
Valenti, S.
Wyatt, S.
Anderson, J. P.
Arcavi, I.
Ashall, C.
Botticella, M. T.
Cartier, R.
Chen, T.-W.
Cikota, A.
Coulter, D.
Valle, M. Della
Foley, R. J.
Gal-Yam, A.
Galbany, L.
Gall, C.
Haislip, J. B.
Harmanen, J.
Hosseinzadeh, G.
Howell, D. A.
Hsiao, Eric
Inserra, C.
Jha, S. W.
Kankare, E.
Kilpatrick, C. D.
Kouprianov, V. V.
Kuncarayakti, Hanindyo
Maccarone, T. J.
Maguire, K.
Mattila, S.
Mazzali, P. A.
McCully, C.
Melandri, A.
Morrell, N.
Phillips, Mark
Pignata, G.
Piro, A. L.
Prentice, S.
Reichart, D. E.
Rojas-Bravo, C.
Smartt, S. J.
Smith, K. W.
Sollerman, J.
Stritzinger, M. D.
Sullivan, M.
Taddia, F.
Young, D. R.
Affiliation
Univ Arizona, Dept AstronUniv Arizona, Steward Observ
Issue Date
2018-01-23Keywords
galaxies: individual (NGC 1532)supernovae: general
supernovae: individual (SN 2016ija, DLT16am)
Metadata
Show full item recordPublisher
IOP PUBLISHING LTDCitation
The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am 2018, 853 (1):62 The Astrophysical JournalJournal
The Astrophysical JournalRights
© 2018. The American Astronomical Society. All rights reserved.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
We present our analysis of the Type II supernova DLT16am (SN 2016ija). The object was discovered during the ongoing D < 40 Mpc (DLT40) one-day cadence supernova search at r similar to 20.1 mag in the "edge-on" nearby (D = 20.0 +/- 4.0 Mpc) galaxy NGC 1532. The subsequent prompt and high-cadenced spectroscopic and photometric follow-up revealed a highly extinguished transient, with E(B - V) = 1.95 +/- 0.15 mag, consistent with a standard extinction law with R-V = 3.1 and a bright (M-V = -18.48 +/- 0.77 mag) absolute peak magnitude. A comparison of the photometric features with those of large samples of SNe II reveals a fast rise for the derived luminosity and a relatively short plateau phase, with a slope of S-50V = 0.84 +/- 0.04 mag/50 days, consistent with the photometric properties typical of those of fast-declining SNe II. Despite the large uncertainties on the distance and the extinction in the direction of DLT16am, the measured photospheric expansion velocity and the derived absolute V-band magnitude at similar to 50 days after the explosion match the existing luminosity-velocity relation for SNe II.ISSN
1538-4357Version
Final published versionSponsors
European Organisation for Astronomical Research in the Southern hemisphere, Chile as part of the ESO large programme [198.A-0915]; Gemini Observatory [GN-2016B-Q-57]; NSF [AST-1412504, AST-1517649, 1313484, AST-1518052]; Carlsberg Foundation; STFC [ST/L000679/1]; EU/FP7-ERC [615929]; Alexander von Humboldt Foundation of Germany; DFG [HA 1850/28-1]; Ministry of Economy, Development, and Tourism's Millennium Science Initiative [IC120009]; Finnish Cultural Foundation; Vilho, Yrjo, and Kalle Vaisala Foundation of the Finnish Academy of Science and Letters; VILLUM FONDEN [13261]; NUTS by the Instrument Center for Danish Astrophysics (IDA); US National Science Foundation [AST-1311862]; National Science Foundation [AST-1008343, AST-1613472, AST-1613426]; EU via ERC grant [725161]; Quantum Universe I-Core program; ISF; BSF Transformative program; Kimmel award; STFC through an Ernest Rutherford Fellowship; Gordon & Betty Moore Foundation; Alfred P. Sloan Foundation; David and Lucile Packard FoundationAdditional Links
http://stacks.iop.org/0004-637X/853/i=1/a=62?key=crossref.ac25350106cfb4c7d554714759f1994bae974a485f413a2113503eed53cd6c53
10.3847/1538-4357/aaa014