The SPIRITS sample of luminous infrared transients: Uncovering hidden supernovae and dusty stellar outbursts in nearby galaxies

Jacob E. Jencson, Mansi M. Kasliwal, Scott M. Adams, Howard E. Bond, Kishalay De, Joel Johansson, Viraj Karambelkar, Ryan M. Lau, Samaporn Tinyanont, Stuart D. Ryder, Ann Marie Cody, Frank J. Masci, John Bally, Nadejda Blagorodnova, Sergio Castellón, Christoffer Fremling, Robert D. Gehrz, George Helou, Charles D. Kilpatrick, Peter A. MilneNidia Morrell, Daniel A. Perley, M. M. Phillips, Nathan Smith, Schuyler D. Van Dyk, Robert Williams

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    We present a systematic study of the most luminous (MIR[Vega magnitudes] brighter than -14) infrared (IR) transients discovered by the SPitzer InfraRed Intensive Transients Survey (SPIRITS) between 2014 and 2018 in nearby galaxies (D < 35 Mpc). The sample consists of nine events that span peak IR luminosities of M[4.5],peakbetween -14 and -18.2, show IR colors between 0.2 < ([3.6]-[4.5]) < 3.0, and fade on timescales between 55 days < t fade< 480 days. The two reddest events (A V > 12) show multiple, luminous IR outbursts over several years and have directly detected, massive progenitors in archival imaging. With analyses of extensive, multiwavelength follow-up, we suggest the following possible classifications: five obscured core-collapse supernovae (CCSNe), two erupting massive stars, one luminous red nova, and one intermediate-luminosity red transient. We define a control sample of all optically discovered transients recovered in SPIRITS galaxies and satisfying the same selection criteria. The control sample consists of eight CCSNe and one Type Iax SN. We find that 7 of the 13 CCSNe in the SPIRITS sample have lower bounds on their extinction of 2 < A V < 8. We estimate a nominal fraction of CCSNe in nearby galaxies that are missed by optical surveys as high as 38.5+26 0%-21.9(90% confidence). This study suggests that a significant fraction of CCSNe may be heavily obscured by dust and therefore undercounted in the census of nearby CCSNe from optical searches.

    Original languageEnglish
    Article number40
    Pages (from-to)1-35
    Number of pages35
    JournalAstrophysical Journal
    Issue number1
    Publication statusPublished - 20 Nov 2019

    Bibliographical note

    Copyright 2019 The American Astronomical Society. First published in the Astrophysical Journal, 886(1), 40, 2019, published by IOP Publishing. The original publication is available at Version archived for private and non-commercial use with the permission of the author/s and according to publisher conditions. For further rights please contact the publisher.


    • dust, extinction
    • infrared: general
    • stars: massive
    • supernovae: general
    • supernovae: individual (SPIRITS 14buu, SPIRITS 15c, SPIRITS 15ud, SPIRITS 16ix, SPIRITS 16tn, SPIRITS 17lb)


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