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Related papers: SN 2002ap, the hypernova of class Ic

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We present the low-resolution spectroscopic and UBVRI broad-band photometric investigations of the Type IIb supernova 2011fu, discovered in UGC 01626. The photometric follow-up of this event has been initiated a few days after the explosion…

We present an extensive set of optical spectroscopy of the nearby type Ia supernova, SN 2002er, with 24 epochs spanning -11 to +34 days. Its spectral evolution is fairly typical of a type Ia supernova although it suffers high extinction.…

We present spectroscopic and photometric data of the Type Ibn supernova (SN) 2014av, discovered by the Xingming Observatory Sky Survey. Stringent pre-discovery detection limits indicate that the object was detected for the first time about…

The recent supernova (SN) known as SN 2009ip had dramatic precursor eruptions followed by an even brighter explosion in 2012. Its pre-2012 observations make it the best documented SN progenitor in history, but have fueled debate about the…

Solar and Stellar Astrophysics · Physics 2015-06-16 Nathan Smith , Jon Mauerhan , Jose Prieto

We present results based on a well sampled optical ($UBVRI$) and ultraviolet ({\it Swift}/UVOT) imaging, and low-resolution optical spectroscopic follow-up observations of the nearby Type Ic supernova (SN) ASASSN-16fp (SN 2016coi). The SN…

High Energy Astrophysical Phenomena · Physics 2017-12-06 Brajesh Kumar , A. Singh , S. Srivastav , D. K. Sahu , G. C. Anupama

We report 139 photometric observations through the B, V, and I filters of the supernova SN 1998bw, an object which is associated with the Gamma-Ray Burst GRB 980425. Detailed light curves of this unique supernova can be compared to…

Astrophysics · Physics 2009-10-31 Eric H. McKenzie , Bradley E. Schaefer

We present UBVRI photometry of the supernova 2011fe in M101, obtained in the interval of 1-652 days after its discovery, as well as one spectrum, taken 105 days after the brightness maximum in the B band. We derived parameters of the light…

Solar and Stellar Astrophysics · Physics 2013-11-15 D. Yu. Tsvetkov , S. Yu. Shugarov , I. M. Volkov , V. P. Goranskij , N. N. Pavlyuk , N. A. Katysheva , E. A. Barsukova , A. F. Valeev

We present optical photometry and spectroscopy of the superluminous SN 2002gh from maximum light to $+204$ days, obtained as part of the Carnegie Type II Supernova (CATS) project. SN 2002gh is among the most luminous discovered supernovae…

Early-time radiative signals from type Ia supernovae (SNe Ia) can provide important constraints on the explosion mechanism and the progenitor system. We present observations and analysis of SN 2019np, a nearby SN Ia discovered within 1-2…

Photometric and spectral evolution of the Type Ic supernova SN 2007ru until around 210 days after maximum are presented. The spectra show broad spectral features due to very high expansion velocity, normally seen in hypernovae. The…

Astrophysics · Physics 2011-02-11 D. K. Sahu , Masaomi Tanaka , G. C. Anupama , Uday K. Gurugubelli , Ken'ichi Nomoto

Optical and ultraviolet observations for the nearby type II-plateau supernova (SN IIP) 2013am in the nearby spiral galaxy M65 are presented in this paper. The early spectra are characterized by relatively narrow P-Cygni features, with…

We present an analysis of the photometric and spectroscopic dataset of the Type II supernova (SN) 2018ivc in the nearby (10 Mpc) galaxy Messier 77. Thanks to the high cadence of the CHASE survey, we observed the SN rising very rapidly by…

The Type Ia supernova (SN Ia) SN 2000cx was one of the most peculiar transients ever discovered, with a rise to maximum brightness typical of a SN Ia, but a slower decline and a higher photospheric temperature. Thirteen years later SN…

We analyze the Type II Plateau supernovae (SN II-P) 2005cs and 2006bp with the non-LTE model atmosphere code CMFGEN. We fit 13 spectra in the first month for SN 2005cs and 18 for SN 2006bp. {\sl Swift} ultraviolet photometry and…

We present highly sampled photometry of the supernova (SN) 2023ixf, a Type II SN in M101, beginning 2 days before its first known detection. To gather these data, we enlisted the global Unistellar Network of citizen scientists. These 252…

High Energy Astrophysical Phenomena · Physics 2023-07-28 Lauren A. Sgro , Thomas M. Esposito , Guillaume Blaclard , Sebastian Gomez , Franck Marchis , Alexei V. Filippenko , Daniel O'Conner Peluso , Stephen S. Lawrence , Aad Verveen , Andreas Wagner , Anouchka Nardi , Barbara Wiart , Benjamin Mirwald , Bill Christensen , Bob Eramia , Bruce Parker , Bruno Guillet , Byungki Kim , Chelsey A. Logan , Christopher C. M. Kyba , Christopher Toulmin , Claudio G. Vantaggiato , Dana Adhis , Dave Gary , Dave Goodey , David Dickinson , David Koster , Davy Martin , Eliud Bonilla , Enner Chung , Eric Miny , Fabrice Mortecrette , Fadi Saibi , Francois O. Gagnon , François Simard , Gary Vacon , Georges Simard , Gerrit Dreise , Hiromi Funakoshi , Janet Vacon , James Yaniz , Jean-Charles Le Tarnec , Jean-Marie Laugier , Jennifer L. W. Siders , Jim Sweitzer , Jiri Dvoracek , John Archer , John Deitz , John K. Bradley , Keiichi Fukui , Kendra Sibbernsen , Kevin Borrot , Kevin Cross , Kevin Heider , Koichi Yamaguchi , Lea A. Hirsch , Liouba Leroux , Mario Billiani , Markus Lorber , Martin J. Smallen , Masao Shimizu , Masayoshi Nishimura , Matthew Ryno , Michael Cunningham , Michael Gagnon , Michael Primm , Michael Rushton , Michael Sibbernsen , Mike Mitchell , Neil Yoblonsky , Niniane Leroux , Olivier Clerget , Ozren Stojanović , Patrice Unique , Patrick Huth , Raymund John Ang , Regis Santoni , Robert Foster , Roberto Poggiali , Ruyi Xu , Ryuichi Kukita , Sanja Šćepanović , Sophie Saibi , Stefan Will , Stephan Latour , Stephen Haythornthwaite , Sylvain Cadieux , Thoralf Müller , Tze Yang Chung , Yoshiya Watanabe , Yvan Arnaud

We present the discovery of a plausible super-luminous supernova (SLSN), found in the archival data of Sloan Digital Sky Survey (SDSS) Stripe 82, called PSN 000123+000504. The supernova peaked at M_g<-21.3 mag in the second half of…

We present an extensive, panchromatic photometric (UV, Optical, and NIR) and low-resolution optical spectroscopic coverage of a Type IIP supernova SN 2018gj that occurred on the outskirts of the host galaxy NGC 6217. From the V-band light…

The Type~Ia supernova (SN~Ia) 2017cfd in IC~0511 (redshift z = 0.01209+- 0.00016$) was discovered by the Lick Observatory Supernova Search 1.6+-0.7 d after the fitted first-light time (FFLT; 15.2 d before B-band maximum brightness).…

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