SPIRITS 15c and SPIRITS 14buu: Two Obscured Supernovae in the Nearby Star-Forming Galaxy IC 2163
arXiv:1609.04444 · doi:10.3847/1538-4357/aa618f
Abstract
SPIRITS---SPitzer InfraRed Intensive Transients Survey---is an ongoing survey of nearby galaxies searching for infrared (IR) transients with Spitzer/IRAC. We present the discovery and follow-up observations of one of our most luminous ( mag, Vega) and red ( mag) transients, SPIRITS 15c. The transient was detected in a dusty spiral arm of IC 2163 ( Mpc). Pre-discovery ground-based imaging revealed an associated, shorter-duration transient in the optical and near-IR (NIR). NIR spectroscopy showed a broad ( km s), double-peaked emission line of He I at m, indicating an explosive origin. The NIR spectrum of SPIRITS 15c is similar to that of the Type IIb SN 2011dh at a phase of days. Assuming mag of extinction in SPIRITS 15c provides a good match between their optical light curves. The IR light curves and the extreme color cannot be explained using only a standard extinction law. Another luminous ( mag) event, SPIRITS 14buu, was serendipitously discovered in the same galaxy. The source displays an optical plateau lasting days, and we suggest a scenario similar to the low-luminosity Type IIP SN 2005cs obscured by mag. Other classes of IR-luminous transients can likely be ruled out in both cases. If both events are indeed SNe, this may suggest of nearby core-collapse SNe are missed by currently operating optical surveys.
arXiv comment19 pages, 7 Figures, 4 Tables
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