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We present optical spectroscopic and photometric observations of the nearby type Ic supernova (SN Ic) SN 2014L. This SN was discovered by the Tsinghua-NAOC Transient Survey (TNTS) in the nearby type-Sc spiral galaxy M99 (NGC 4254). Fitting…

Extensive optical and near-infrared (NIR) observations of the type Ib supernova 1999dn are presented, covering the first year after explosion. These new data turn this object, already considered a prototypical SNIb, into one of the best…

We present a sample of 14 hydrogen-rich superluminous supernovae (SLSNe II) from the Zwicky Transient Facility (ZTF) between 2018 and 2020. We include all classified SLSNe with peaks $M_{g}<-20$ mag and with observed \emph{broad} but not…

We present nebular spectra of the Type Ia supernova (SN Ia) SN 2019yvq, which had a bright flash of blue and ultraviolet light after exploding, followed by a rise similar to other SNe Ia. Although SN 2019yvq displayed several other rare…

High Energy Astrophysical Phenomena · Physics 2021-03-22 Matthew R. Siebert , Georgios Dimitriadis , Abigail Polin , Ryan J. Foley

We present new photometric and spectroscopic observations of SN 2019yvq, a Type Ia supernova (SN Ia) exhibiting several peculiar properties including an excess of UV/optical flux within days of explosion, a high SiII velocity, and a low…

High Energy Astrophysical Phenomena · Physics 2021-07-20 M. A. Tucker , C. Ashall , B. J. Shappee , P. J. Vallely , C. S. Kochanek , M. E. Huber , G. S. Anand , J. V. Keane , E. Y. Hsiao , T. W. -S. Holoien

We present photometric and spectroscopic observations of the Type Icn supernova (SN) 2021ckj. Spectral modeling of SN 2021ckj reveals that its composition is dominated by oxygen, carbon and iron group elements, and the photospheric velocity…

We present Keck optical spectra of SN 2002cx, the most peculiar known Type Ia supernova (SN Ia), taken 227 and 277 days past maximum light. Astonishingly, the spectra are not dominated by the forbidden emission lines of iron that are a…

We present the results of low-resolution spectroscopic and densely sampled multi-band photometric follow-up of supernova (SN) 2024aecx. The SN was discovered in the spiral galaxy NGC 3521 (distance $\sim$11 Mpc) within a day after the…

Optical and near-infrared observations of the Type Ic supernova (SN) 2004aw are presented, obtained from day -3 to day +413 with respect to the B-band maximum. The photometric evolution is characterised by a comparatively slow post-maximum…

We analyse the early-time optical light curves (LCs) of 20 Type Ib/c supernovae (SNe Ib/c) from the Sloan Digital Sky Survey (SDSS) SN survey II, aiming to study their properties as well as to derive their progenitor parameters.…

High Energy Astrophysical Phenomena · Physics 2015-01-28 F. Taddia , J. Sollerman , G. Leloudas , M. D. Stritzinger , S. Valenti , L. Galbany , R. Kessler , D. P. Schneider , J. C. Wheeler

Stripped-envelope core-collapse supernovae can be divided into two broad classes: the common Type Ib/c supernovae (SNe Ib/c), powered by the radioactive decay of $^{56}$Ni, and the rare superluminous supernovae (SLSNe), most likely powered…

High Energy Astrophysical Phenomena · Physics 2022-12-21 Sebastian Gomez , Edo Berger , Matt Nicholl , Peter K. Blanchard , Griffin Hosseinzadeh

We present an exquisite, 30-min cadence Kepler (K2) light curve of the Type Ia supernova (SN Ia) 2018oh (ASASSN-18bt), starting weeks before explosion, covering the moment of explosion and the subsequent rise, and continuing past peak…

High Energy Astrophysical Phenomena · Physics 2019-01-09 G. Dimitriadis , R. J. Foley , A. Rest , D. Kasen , A. L. Piro , A. Polin , D. O. Jones , A. Villar , G. Narayan , D. A. Coulter , C. D. Kilpatrick , Y. -C. Pan , C. Rojas-Bravo , O. D. Fox , S. W. Jha , P. E. Nugent , A. G. Riess , D. Scolnic , M. R. Drout , G. Barentsen , J. Dotson , M. Gully-Santiago , C. Hedges , A. M. Cody , T. Barclay , S. Howell , P. Garnavich , B. E. Tucker , E. Shaya , R. Mushotzky , R. P. Olling , S. Margheim , A. Zenteno , J. Coughlin , J. E. Van Cleve , J. Vinicius de Miranda Cardoso , K. A. Larson , K. M. McCalmont-Everton , C. A. Peterson , S. E. Ross , L. H. Reedy , D. Osborne , C. McGinn , L. Kohnert , L. Migliorini , A. Wheaton , B. Spencer , C. Labonde , G. Castillo , G. Beerman , K. Steward , M. Hanley , R. Larsen , R. Gangopadhyay , R. Kloetzel , T. Weschler , V. Nystrom , J. Moffatt , M. Redick , K. Griest , M. Packard , M. Muszynski , J. Kampmeier , R. Bjella , S. Flynn , B. Elsaesser , K. C. Chambers , H. A. Flewelling , M. E. Huber , E. A. Magnier , C. Z. Waters , A. S. B. Schultz , J. Bulger , T. B. Lowe , M. Willman , S. J. Smartt , K. W. Smith , S. Points , G. M. Strampelli , J. Brimacombe , P. Chen , J. A. Munoz , R. L. Mutel , J. Shields , P. J. Vallely , S. Villanueva , W. Li , X. Wang , J. Zhang , H. Lin , J. Mo , X. Zhao , H. Sai , X. Zhang , K. Zhang , T. Zhang , L. Wang , J. Zhang , E. Baron , J. M. DerKacy , L. Li , Z. Chen , D. Xiang , L. Rui , L. Wang , F. Huang , X. Li , G. Hosseinzadeh , D. A. Howell , I. Arcavi , D. Hiramatsu , J. Burke , S. Valenti , J. L. Tonry , L. Denneau , A. N. Heinze , H. Weiland , B. Stalder , J. Vinko , K. Sarneczky , A. Pa , A. Bodi , Zs. Bognar , B. Csak , B. Cseh , G. Csornyei , O. Hanyecz , B. Ignacz , Cs. Kalup , R. Konyves-Toth , L. Kriskovics , A. Ordasi , I. Rajmon , A. Sodor , R. Szabo , R. Szakats , G. Zsidi , S. C. Williams , J. Nordin , R. Cartier , C. Frohmaier , L. Galbany , C. P. Gutierrez , I. Hook , C. Inserra , M. Smith , D. J. Sand , J. E. Andrews , N. Smith , C. Bilinski

We present extensive multi-wavelength observations of the extremely rapidly declining Type Ic supernova, SN 2005ek. Reaching a peak magnitude of M_R = -17.3 and decaying by ~3 mag in the first 15 days post-maximum, SN 2005ek is among the…

SN2018ibb is a recently observed hydrogen poor super-luminous supernova which appears to be powered by the decay of $30\;\rm{M_\odot}$ of radioactive nickel. This supernova has been suggested to show hybrid signatures of a pair instability…

High Energy Astrophysical Phenomena · Physics 2024-07-18 Chris Nagele , Hideyuki Umeda , Keiichi Maeda

We present a detailed spectroscopic analysis of the recently discovered fast evolving Type I superluminous supernova (SLSN-I), SN 2019neq (at redshift z = 0.1059) comparing it to the well-studied slow evolving SLSN-I, SN 2010kd (z = 0.101).…

High Energy Astrophysical Phenomena · Physics 2020-09-09 R. Konyves-Toth , B. P. Thomas , J. Vinko , J. C. Wheeler

We present SN 2019tsf (ZTF19ackjszs) and SN 2019oys (ZTF19abucwzt). These two stripped envelope Type Ib supernovae suddenly showed a (re-)brightening in their late light curves. We investigate this in the context of circumstellar material…

The optical observations of Ic-4 supernova (SN) 2016coi/ASASSN-16fp, from $\sim 2$ to $\sim450$ days after explosion, are presented along with analysis of its physical properties. The SN shows the broad lines associated with SNe Ic-3/4 but…

We report the first detection of a credible progenitor system for a Type Ic supernova (SN Ic), SN 2017ein. We present spectra and photometry of the SN, finding it to be similar to carbon-rich, low-luminosity SNe Ic. Using a post-explosion…

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