On the Ca-strong 1991bg-like type Ia supernova 2016hnk: evidence for a Chandrasekhar-mass explosion

22 Apr 2019Lluís GalbanyChris AshallPeter HoeflichSantiago González-GaitánStefan TaubenbergerMaximilian StritzingerEric Y. HsiaoPaolo MazzaliEddie BaronStéphane BlondinSubhash BoseMattia BullaJamison F. BurkeChristopher R. BurnsRégis CartierPing ChenMassimo Della ValleTiara R. DiamondClaudia P. GutiérrezJussi HarmanenDaichi HiramatsuT. W. -S. HoloienGriffin HosseinzadehD. Andrew HowellYiwen HuangCosimo InserraThomas de JaegerSaurabh W. JhaTuomas KangasMarkus KromerJoseph D. LymanKate MaguireGeorge Howie MarionDan MilisavljevicSimon J. PrenticeAlessandro RazzaThomas M. ReynoldsDavid J. SandBenjamin J. ShappeeRohit ShekharStephen J. SmarttKeivan G. StassunMark SullivanStefano ValentiSteven VillanuevaXiaofeng WangJ. Craig WheelerQian ZhaiJujia Zhang

We present a comprehensive dataset of optical and near-infrared photometry and spectroscopy of type~Ia supernova (SN) 2016hnk, combined with integral field spectroscopy (IFS) of its host galaxy, MCG -01-06-070, and nearby environment. Properties of the SN local environment are characterized by means of single stellar population synthesis applied to IFS observations taken two years after the SN exploded... (read more)

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