Early-time light curves of Type Ib/c supernovae from the SDSS-II Supernova Survey

2014/08/31 by F. Taddia, J. Sollerman, G. Leloudas +6 · 4 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Gamma-ray bursts and supernovae #Homogeneous #Light curve #Phase (matter) #Stellar, planetary, and galactic studies #Supernova #Type (biology) #Type II supernova #astro-ph.CO #astro-ph.HE #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201423915

published as A&A 574, A60 (2015) · Replaced to match the accepted version. The abstract was shortened by 30% to fit the arXiv limits

arxiv created 2014/11/07 · openalex publication_date 2015/01/26 · arxiv updated 2015/01/28 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. Type Ib/c supernovae (SNe Ib/c) have been investigated in several single-object studies; however, there is still a paucity of works concerning larger, homogeneous samples of these hydrogen-poor transients, in particular regarding the premaximum phase of their light curves.

Citations

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• Investigating the observational properties of Type Ib supernova SN 2017iro
• Analyzing the Largest Spectroscopic Data Set of Hydrogen-poor Super-luminous Supernovae
• Studying the environment of AT 2018cow with MUSE