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Related papers: SN 2008S: an electron capture SN from a super-AGB …

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A set of hydrodynamical models based on stellar evolutionary progenitors is used to study the nature of SN 2011dh. Our modeling suggests that a large progenitor star ---with R ~200 Rsun---, is needed to reproduce the early light curve of SN…

We use the progenitor of SN2012aw to illustrate the consequences of modeling circumstellar dust using Galactic (interstellar) extinction laws that (1) ignore dust emission in the near-IR and beyond; (2) average over dust compositions, and…

Solar and Stellar Astrophysics · Physics 2015-06-11 C. S. Kochanek , R. Khan , X. Dai

We propose an alternative explanation for the post-breakout emission of SN 2008D associated with the X-ray transient 080109. Observations of this object show a very small contrast of 0.35 dex between the light-curve minimum occurring soon…

Solar and Stellar Astrophysics · Physics 2015-06-15 Melina C. Bersten , Masaomi Tanaka , Nozomu Tominaga , Omar G. Benvenuto , Ken'ichi Nomoto

We perform hydrodynamical calculations of core-collapse supernovae (SNe) with low explosion energies. These SNe do not have enough energy to eject the whole progenitor and most of the progenitor falls back to the central remnant. We show…

High Energy Astrophysical Phenomena · Physics 2010-08-02 Takashi Moriya , Nozomu Tominaga , Masaomi Tanaka , Ken'ichi Nomoto , Daniel N. Sauer , Paolo A. Mazzali , Keiichi Maeda , Tomoharu Suzuki

The galaxy SDSSJ0952+2143 showed remarkable emission-line properties first reported in 2008 (paper I), which are the consequence of a powerful high-energy flare. Here we report follow-up observations of SDSSJ0952+2143, and discuss outburst…

Astrophysics of Galaxies · Physics 2009-07-24 S. Komossa , H. Zhou , A. Rau , M. Dopita , A. Gal-Yam , J. Greiner , J. Zuther , M. Salvato , D. Xu , H. Lu , R. Saxton , M. Ajello

We present photometric and spectroscopic observations of SN 2013fc, a bright type II supernova (SN) in a circumnuclear star-forming ring in the luminous infrared galaxy ESO 154-G010, observed as part of the Public ESO Spectroscopic Survey…

Extensive photometric and spectroscopic observations of SN1994aj until 540d after maximum light have been obtained. The photometry around maximum suggests that the SN belongs to the Type II Linear class, with a peak absolute magnitude of Mv…

Astrophysics · Physics 2020-11-25 S. Benetti , E. Cappellaro , I. J. Danziger , M. Turatto , F. Patat , M. Della Valle

We report the identification of a source coincident with SN 2009kr in HST pre-explosion images. The object appears to be a single point source with an intrinsic colour V-I = 1.1 and M_V = -7.6. If this is a single star it would be a yellow…

We report extensive radio and X-ray observations of SN 2003bg whose spectroscopic evolution shows a transition from a broad-lined Type Ic to a hydrogen-rich Type II and later to a typical hydrogen-poor Type Ibc. We show that the…

Astrophysics · Physics 2008-11-26 A. M. Soderberg , R. A. Chevalier , S. R. Kulkarni , D. A. Frail

Supernova (SN) 2004et is the eighth historical SN in the nearby spiral galaxy NGC 6946. Here we report on early photometric and spectroscopic monitoring of this object. SN 2004et is a Type II event, exhibiting a plateau in its light curves,…

Context: SN 2024ggi is a Type II supernova (SN) discovered in the nearby galaxy NGC 3621 (D $\approx6.7\pm0.d$ Mpc) on 2024 April 03.21 UT. Its proximity enabled a detailed investigation of the SN's properties and its progenitor star. This…

We present results of a search for a supernova (SN) component associated with GRB 100418A at the redshift of 0.624. The field of GRB 100418A was observed with FOCAS on Subaru 8.2m telescope under a photometric condition (seeing 0.3"-0.4")…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Yuu Niino , Tetsuya Hashimoto , Kentaro Aoki , Takashi Hattori , Kiyoto Yabe , Ken'ichi Nomoto

We present new light curves and spectra for a number of extragalactic optical transients or "SN impostors" related to giant eruptions of LBVs, and we provide a comparative discussion of LBV-like giant eruptions known to date. New data…

Solar and Stellar Astrophysics · Physics 2015-05-20 Nathan Smith , Weidong Li , Jeffrey M. Silverman , Mo Ganeshalingam , Alexei V. Filippenko

We present the spectroscopic discovery of a broad-lined Type Ic supernova (SN 2010bh) associated with the nearby long-duration gamma-ray burst (GRB) 100316D. At z = 0.0593, this is the third-nearest GRB-SN. Nightly optical spectra obtained…

We follow our first paper with an analysis of the ensemble of the extensive pre-explosion ground- and space-based infrared observations of the red supergiant (RSG) progenitor candidate for the nearby core-collapse supernova SN 2023ixf in…

As part of the European Supernova Collaboration we obtained extensive photometry and spectroscopy of the type Ia SN 2002dj covering epochs from 11 days before to nearly two years after maximum. Detailed optical and near-infrared…

We present new HST imaging photometry for the site of the Type IIn supernova (SN) 2009ip taken almost a decade after explosion. The optical source has continued to fade steadily since the SN-like event in 2012. In the F606W filter, which…

High Energy Astrophysical Phenomena · Physics 2022-06-29 Nathan Smith , Jennifer E. Andrews , Alexei V. Filippenko , Ori D. Fox , Jon C. Mauerhan , Schuyler D. Van Dyk

We present optical photometry and spectroscopy of SN 2016iet, an unprecedented Type I supernova (SN) at $z=0.0676$ with no obvious analog in the existing literature. The peculiar light curve has two roughly equal brightness peaks ($\approx…

We present Hubble Space Telescope imaging of a pre-explosion counterpart to SN 2019yvr obtained 2.6 years before its explosion as a type Ib supernova (SN Ib). Aligning to a post-explosion Gemini-S/GSAOI image, we demonstrate that there is a…