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19982024
most citedSpectroscopic Discovery of the Supernova 2003dh Associated with GRB 030329

1.2k citations · 8.9k across the 90 of their papers we have counts for

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Showing astro-ph.COShow all

5 papers · 1 filter

astro-ph.CO2015★ 77 cited

The Young and Bright Type Ia Supernova ASASSN-14lp: Discovery, Early-Time Observations, First-Light Time, Distance to NGC 4666, and Progenitor Constraints

B. J. Shappee, A. L. Piro, T. W. -S. Holoien +29

On 2014 Dec. 9.61, the All-Sky Automated Survey for SuperNovae (ASAS-SN or "Assassin") discovered ASASSN-14lp just days after first light using a global array of 14-cm diam…

astro-ph.CO2012★ 58 cited

Discovery and Early Multi-Wavelength Measurements of the Energetic Type Ic Supernova PTF12gzk: A Massive-Star Explosion in a Dwarf Host Galaxy

Sagi Ben-Ami, Avishay Gal-Yam, Alexei V. Filippenko +45

We present the discovery and extensive early-time observations of the Type Ic supernova (SN) PTF12gzk. Our finely sampled light curves show a rise of 0.8mag within 2.5hr. Power-law…

astro-ph.CO2011★ 510 cited

Supernova 2011fe from an Exploding Carbon-Oxygen White Dwarf Star

Peter E. Nugent, Mark Sullivan, S. Bradley Cenko +36

Type Ia supernovae (SNe Ia) have been used empirically as standardized candles to reveal the accelerating universe even though fundamental details, such as the nature of the progen…

astro-ph.CO2011★ 106 cited

Real-Time Detection and Rapid Multiwavelength Follow-up Observations of a Highly Subluminous Type II-P Supernova from the Palomar Transient Factory Survey

Avishay Gal-Yam, Mansi M. Kasliwal, Iair Arcavi +29

The Palomar Transient Factory (PTF) is an optical wide-field variability survey carried out using a camera with a 7.8 square degree field of view mounted on the 48-in Oschin Schmid…

astro-ph.CO2010★ 225 cited

Discovery of the nearby long, soft GRB 100316D with an associated supernova

R. L. C. Starling, K. Wiersema, A. J. Levan +43

We report the Swift discovery of nearby long, soft gamma-ray burst GRB 100316D, and the subsequent unveiling of its low redshift host galaxy and associated supernova. We derive the…