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Related papers: DES16C3cje: A low-luminosity, long-lived supernova

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Current large-scale, high-cadence surveys, such as the ZTF, provide detections of new and rare types of transients and supernovae whose physical origins are not well understood. We investigate the nature of SN 2021lwz at a redshift…

We present observations of two new hydrogen-poor superluminous supernovae (SLSN-I), iPTF15esb and iPTF16bad, showing late-time H-alpha emission with line luminosities of (1-3)e+41 erg/s and velocity widths of (4000-6000) km/s. Including the…

Type Iax supernovae represent the largest class of peculiar white-dwarf supernovae. The type Iax SN~2012Z in NGC 1309 is the only white dwarf supernova with a detected progenitor system in pre-explosion observations. Deep \textit{Hubble…

Hydrogen-rich Type II supernovae (SNe II) are the most frequently observed class of core-collapse SNe (CCSNe). However, most studies that analyse large samples of SNe II lack events with absolute peak magnitudes brighter than -18.5 mag at…

We present optical photometry and spectroscopy of the Type IIn supernova (SN) 2021qqp. Its unusual light curve is marked by a long precursor for $\approx300$ days, a rapid increase in brightness for $\approx60$ days, and then a sharp…

The Gamma-Ray Burst 031203 at a redshift z=0.1055 revealed a highly reddened Type Ic Supernova, SN 2003lw, in its afterglow light. This is the third well established case of a link between a long-duration GRB and a type Ic SN. The SN light…

We present spectra and lightcurves of SNLS 06D4eu and SNLS 07D2bv, two hydrogen-free superluminous supernovae discovered by the Supernova Legacy Survey. At z = 1.588, SNLS 06D4eu is the highest redshift superluminous SN with a spectrum, at…

We present optical and near-infrared light curves of SN 2001el from 310 to 445 days past maximum light, obtained with the Very Large Telescope. The late-time optical (UBVRI) light curves decay in a nearly linear fashion with decay time…

Astrophysics · Physics 2009-11-13 Maximilian Stritzinger , Jesper Sollerman

We present a comprehensive data set of supernova (SN) 2016adj located within the central dust lane of Centaurus A. SN 2016adj is significantly reddened and after correcting the peak apparent $B$-band magnitude ($m_B = 17.48\pm0.05$) for…

We present comprehensive photometric and spectroscopic observations of Supernova (SN) 2022eyw, a luminous member of the Type Iax SN subclass. SN 2022eyw reached a peak absolute magnitude of $M_g = -17.80\pm0.15$ mag and exhibited a rise…

High Energy Astrophysical Phenomena · Physics 2026-03-03 Hrishav Das , Devendra K. Sahu , Anirban Dutta , Mridweeka Singh , G. C. Anupama , Rishabh Singh Teja

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 calculate the volumetric rate of superluminous supernovae (SLSNe) based on 5 events discovered with the ROTSE-IIIb telescope. We gather light curves of 19 events from the literature and our own unpublished data and employ crude…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 Robert M. Quimby , Fang Yuan , Car Akerlof , J. Craig Wheeler

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).…

We present optical photometric and spectroscopic observations of the Type~IIb supernova (SN)~2017ati. It reached the maximum light at about 27~d after the explosion and the light curve shows a broad, luminous peak with an absolute $r$-band…

We present optical, infrared, ultraviolet, and radio observations of SN 2022xkq, an underluminous fast-declining type Ia supernova (SN Ia) in NGC 1784 ($\mathrm{D}\approx31$ Mpc), from $<1$ to 180 days after explosion. The high-cadence…

High Energy Astrophysical Phenomena · Physics 2023-10-10 Jeniveve Pearson , David J. Sand , Peter Lundqvist , Lluís Galbany , Jennifer E. Andrews , K. Azalee Bostroem , Yize Dong , Emily Hoang , Griffin Hosseinzadeh , Daryl Janzen , Jacob E. Jencson , Michael J. Lundquist , Darshana Mehta , Nicolás Meza Retamal , Manisha Shrestha , Stefano Valenti , Samuel Wyatt , Joseph P. Anderson , Chris Ashall , Katie Auchettl , Eddie Baron , Stéphane Blondin , Christopher R. Burns , Yongzhi Cai , Ting-Wan Chen , Laura Chomiuk , David A. Coulter , Dane Cross , Kyle W. Davis , Thomas de Jaeger , James M. DerKacy , Dhvanil D. Desai , Georgios Dimitriadis , Aaron Do , Joseph R. Farah , Ryan J. Foley , Mariusz Gromadzki , Claudia P. Gutiérrez , Joshua Haislip , Jonay I. González Hernández , Jason T. Hinkle , Willem B. Hoogendam , D. Andrew Howell , Peter Hoeflich , Eric Hsiao , Mark E. Huber , Saurabh W. Jha , Cristina Jiménez Palau , Charles D. Kilpatrick , Vladimir Kouprianov , Sahana Kumar , Lindsey A. Kwok , Conor Larison , Natalie LeBaron , Xavier Le Saux , Jing Lu , Curtis McCully , Tycho Mera Evans , Peter Milne , Maryam Modjaz , Nidia Morrell , Tomás E. Müller-Bravo , Megan Newsome , Matt Nicholl , Estefania Padilla Gonzalez , Anna V. Payne , Craig Pellegrino , Kim Phan , Jonathan Pineda-García , Anthony L. Piro , Lara Piscarreta , Abigail Polin , Daniel E. Reichart , César Rojas-Bravo , Stuart D. Ryder , Irene Salmaso , Michaela Schwab , Melissa Shahbandeh , Benjamin J. Shappee , Matthew R. Siebert , Nathan Smith , Jay Strader , Kirsty Taggart , Giacomo Terreran , Samaporn Tinyanont , M. A. Tucker , Giorgio Valerin , D. R. Young

We present new data for five under-luminous type II-plateau supernovae (SNe IIP), namely SN 1999gn, SN 2002gd, SN 2003Z, SN 2004eg and SN 2006ov. This new sample of low-luminosity SNe IIP (LL SNe IIP) is analyzed together with similar…

We investigate the use of type Ic Super Luminous Supernovae as standardizable candles and distance indicators. Their appeal as cosmological probes stems from their remarkable peak luminosities, hot blackbody temperatures and bright…

Solar and Stellar Astrophysics · Physics 2015-06-22 Cosimo Inserra , Stephen J. Smartt

We present VRIJHK photometry, and optical and near-infrared spectroscopy, of the heavily extinguished Type Ia supernova (SN) 2002cv, located in NGC 3190, which is also the parent galaxy of the Type Ia SN 2002bo. SN 2002cv, not visible in…

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