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We identify the progenitor star of SN 2023ixf in the nearby galaxy Messier 101 using Keck/NIRC2 adaptive optics imaging and pre-explosion HST/ACS images. The supernova position, localized with diffraction-spike pattern and high precision…

We present and analyze observations of the Type Ib supernova (SN) 2019odp (a.k.a ZTF19abqwtfu) covering epochs within days of the explosion to the nebular phase at 360 d post-explosion. We discuss them in the context of recombination…

Recent evidence of a young progenitor population for many Type-Ia SNe (SNe-Ia) raises the possibility that evolved intermediate-mass progenitor stars may be detected in pre-explosion images. NGC 1316, a radio galaxy in the Fornax cluster,…

Astrophysics · Physics 2009-11-13 Dan Maoz , Filippo Mannucci

We report the results of our search for the progenitor candidate of SN 2013dk, a Type Ic supernova (SN) that exploded in the Antennae Galaxy system. We compare pre-explosion Hubble Space Telescope (HST) archival images with SN images…

We present the identification of the progenitor of the Type IIP SN 2012ec in archival pre-explosion HST WFPC2 and ACS/WFC F814W images. The properties of the progenitor are further constrained by non-detections in pre-explosion WFPC2 F450W…

Hubble Space Telescope observations of the site of the supernova (SN) 2008ax obtained in 2011 and 2013 reveal that the possible progenitor object detected in pre-explosion images was in fact multiple. Four point sources are resolved in the…

Solar and Stellar Astrophysics · Physics 2015-10-07 Gastón Folatelli , Melina C. Bersten , Hanindyo Kuncarayakti , Omar G. Benvenuto , Keiichi Maeda , Ken'ichi Nomoto

Type IIb Supernova (SN) 2011dh, with conclusive detection of an unprecedented Yellow Supergiant (YSG) progenitor, provides an excellent opportunity to deepen our understanding on the massive star evolution in the final centuries toward the…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Keiichi Maeda , Satoru Katsuda , Aya Bamba , Yukikatsu Terada , Yasushi Fukazawa

We present six epochs of spectropolarimetric observations and one epoch of spectroscopy of the Type Ib SN iPTF 13bvn. The epochs of these observations correspond to $-$10 to $+$61 days with respect to the {\it r}-band light curve maximum.…

A Type IIn supernova (SN) is dominated by the interaction of SN ejecta with the circumstellar medium (CSM). Some SNe IIn (e.g., SN 2006jd) have episodes of re-brightening ("bumps") in their light curves. We present iPTF13z, a SN IIn…

Solar and Stellar Astrophysics · Physics 2017-09-21 A. Nyholm , J. Sollerman , F. Taddia , C. Fremling , T. J. Moriya , E. O. Ofek , A. Gal-Yam , A. De Cia , R. Roy , M. M. Kasliwal , Y. Cao , P. E. Nugent , F. J. Masci

Type IIb supernovae (SNe) are a transitional subclass of stripped-envelope SNe showing hydrogen lines in their spectra that gradually weaken and give way to helium lines reminiscent of SNe Ib, which is indicative of stripping through…

High Energy Astrophysical Phenomena · Physics 2026-01-14 S. de Wet , G. Leloudas , D. Buckley , N. Erasmus , P. J. Groot , E. Zimmerman

This Letter presents the detection of a source at the position of the Type Ib/c supernova (SN) 2013ge more than four years after the radioactive component is expected to have faded. This source could mark the first post-SN direct detection…

Over the last 15 years, the supernova community has endeavoured to identify progenitor stars of core-collapse supernovae in high resolution archival images of their galaxies.This review compiles results (from 1999 - 2013) in a distance…

Solar and Stellar Astrophysics · Physics 2015-05-12 S. J. Smartt

The progenitors of many Type II supernovae have been observationally identified but the search for Type Ibc supernova (SN Ibc) progenitors has thus far been unsuccessful, despite the expectation that they are luminous Wolf-Rayet (WR) stars.…

Solar and Stellar Astrophysics · Physics 2015-06-05 S. -C. Yoon , G. Graefener , J. S. Vink , A. Kozyreva , R. G. Izzard

In BTA spectra of the supernova SN2006aj, identified with the X-ray flash (XRF) and gamma-ray burst XRF/GRB060218/SN2006aj, we detected details interpreted as hydrogen lines, which is a sign of stellar-wind envelope around a massive…

Models for the spectra and the light curve, in the photospheric as well as in the late nebular phase, are used to infer the properties of the very radio-bright, broad-lined type IIb Supernova 2003bg. Consistent fits to the light curve and…

High Energy Astrophysical Phenomena · Physics 2015-05-13 Paolo A. Mazzali , Jinsong Deng , Mario Hamuy , Ken'ichi Nomoto

We present high quality ground-based VRI images of the site of the Type II-P SN1999em (in NGC1637) taken before explosion, which were extracted from the CFHT archive. We determine a precise position of the SN on these images to an accuracy…

Astrophysics · Physics 2009-11-06 S. J. Smartt , G. F. Gilmore , C. A. Tout , S. T. Hodgkin

Context. Type Ibn supernovae (SNe) are characterized by narrow helium emission lines arising from ejecta-circumstellar medium interaction, yet their progenitors remain debated, with both massive Wolf-Rayet stars and low-mass helium stars in…

Solar and Stellar Astrophysics · Physics 2026-05-25 Xinyi Hong , Ning-Chen Sun , Yali Shao , Ke Wang , Junjie Wu , Qiang Xi , Yi-Han Zhao , Justyn Maund , Xiaohan Chen , Anyu Wang , Linxi Zhang , Jifeng Liu

We present spectroscopic and photometric observations and analysis of SN 2024abvb, a peculiar transitional Type Ibn/Icn supernova located at an unusually large projected distance from its host galaxy (21.5 kpc). SN 2024abvb displays an…

The Type IIb supernova (SN) 1993J is one of only a few stripped-envelope supernovae with a progenitor star identified in pre-explosion images. SN IIb models typically invoke H envelope stripping by mass transfer in a binary system. For the…

We present optical photometric and spectroscopic observations of the Type Ibn (SN 2006jc-like) supernova iPTF13beo. Detected by the intermediate Palomar Transient Factory ~3 hours after the estimated first light, iPTF13beo is the youngest…