The HSC-SSP Transient Survey: Implications from Early Photometry and Rise Time of Normal Type Ia Supernovae

Ji An Jiang, Naoki Yasuda, Keiichi Maeda, Mamoru Doi, Toshikazu Shigeyama, Nozomu Tominaga, Masaomi Tanaka, Takashi J. Moriya, Ichiro Takahashi, Nao Suzuki, Tomoki Morokuma, Ken'ichi Nomoto

Research output: Contribution to journalArticlepeer-review

5 Citations (Scopus)

Abstract

With a booming number of Type Ia supernovae (SNe Ia) discovered within a few days of their explosions, a fraction of SNe Ia that show luminosity excess in the early phase (early-excess SNe Ia) have been confirmed. In this article, we report early-phase observations of seven photometrically normal SNe Ia (six early detections and one deep non detection limit) at the COSMOS field through a half-year transient survey as a part of the Hyper Suprime-Cam Subaru Strategic Program (HSC SSP). In particular, a blue light-curve excess was discovered for HSC17bmhk, a normal SN Ia with rise time longer than 18.8 days, during the first four days after the discovery. The blue early excess in optical wavelength can be explained not only by interactions with a nondegenerate companion or surrounding dense circumstellar matter but also radiation powered by radioactive decays of 56Ni at the surface of the SN ejecta. Given the growing evidence of the early-excess discoveries in normal SNe Ia that have longer rise times than the average, and a similarity in the nature of the blue excess to a luminous SN Ia subclass, we infer that early excess discovered in HSC17bmhk and other normal SNe Ia are most likely attributed to radioactive 56Ni decay at the surface of the SN ejecta. In order to successfully identify normal SNe Ia with early excess similar to that of HSC17bmhk, early UV photometries or high-cadence blue-band surveys are necessary.

Original languageEnglish
Article number25
JournalAstrophysical Journal
Volume892
Issue number1
DOIs
Publication statusPublished - 2020 Mar 20

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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