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    The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am

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    Author
    Tartaglia, L. cc
    Sand, David J. cc
    Valenti, S. cc
    Wyatt, S.
    Anderson, J. P.
    Arcavi, I. cc
    Ashall, C.
    Botticella, M. T.
    Cartier, R.
    Chen, T.-W. cc
    Cikota, A. cc
    Coulter, D. cc
    Valle, M. Della cc
    Foley, R. J.
    Gal-Yam, A. cc
    Galbany, L.
    Gall, C.
    Haislip, J. B.
    Harmanen, J.
    Hosseinzadeh, G. cc
    Howell, D. A. cc
    Hsiao, Eric cc
    Inserra, C. cc
    Jha, S. W. cc
    Kankare, E.
    Kilpatrick, C. D.
    Kouprianov, V. V.
    Kuncarayakti, Hanindyo cc
    Maccarone, T. J.
    Maguire, K.
    Mattila, S.
    Mazzali, P. A. cc
    McCully, C. cc
    Melandri, A.
    Morrell, N.
    Phillips, Mark cc
    Pignata, G. cc
    Piro, A. L.
    Prentice, S.
    Reichart, D. E. cc
    Rojas-Bravo, C.
    Smartt, S. J. cc
    Smith, K. W.
    Sollerman, J. cc
    Stritzinger, M. D.
    Sullivan, M. cc
    Taddia, F.
    Young, D. R.
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    Affiliation
    Univ Arizona, Dept Astron
    Univ Arizona, Steward Observ
    Issue Date
    2018-01-23
    Keywords
    galaxies: individual (NGC 1532)
    supernovae: general
    supernovae: individual (SN 2016ija, DLT16am)
    
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    Publisher
    IOP PUBLISHING LTD
    Citation
    The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am 2018, 853 (1):62 The Astrophysical Journal
    Journal
    The Astrophysical Journal
    Rights
    © 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
    1538-4357
    DOI
    10.3847/1538-4357/aaa014
    Version
    Final published version
    Sponsors
    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 Foundation
    Additional Links
    http://stacks.iop.org/0004-637X/853/i=1/a=62?key=crossref.ac25350106cfb4c7d554714759f1994b
    ae974a485f413a2113503eed53cd6c53
    10.3847/1538-4357/aaa014
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