activity
20092024
most citedSpectra of Hydrogen-Poor Superluminous Supernovae from the Palomar Transient Factory

140 citations · 906 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2024★ 6 cited

SN 2023zaw: an ultra-stripped, nickel-poor supernova from a low-mass progenitor

Kaustav K. Das, Christoffer Fremling, Mansi M. Kasliwal +34

We present SN 2023zaw a sub-luminous ( mag) and rapidly-evolving supernova ( days), with the lowest nickel mass (…

astro-ph.SR2020★ 42 cited

Berkeley Supernova Ia Program: Data Release of 637 Spectra from 247 Type Ia Supernovae

Benjamin E. Stahl, WeiKang Zheng, Thomas de Jaeger +18

We present 637 low-redshift optical spectra collected by the Berkeley Supernova Ia Program (BSNIP) between 2009 and 2018, almost entirely with the Kast double spectrograph on the S…

astro-ph.SR2019★ 83 cited

Lick Observatory Supernova Search Follow-Up Program: Photometry Data Release of 93 Type Ia Supernovae

Benjamin E. Stahl, WeiKang Zheng, Thomas de Jaeger +52

We present BVRI and unfiltered light curves of 93 Type Ia supernovae (SNe Ia) from the Lick Observatory Supernova Search (LOSS) follow-up program conducted between 2005 and 2018. O…

astro-ph.SR2018★ 93 cited

The Berkeley Sample of Stripped-Envelope Supernovae

Isaac Shivvers, Alexei V. Filippenko, Jeffrey M. Silverman +22

We present the complete sample of stripped-envelope supernova (SN) spectra observed by the Lick Observatory Supernova Search (LOSS) collaboration over the last three decades: 888 s…

astro-ph.HE2018★ 20 cited

Helium giant stars as progenitors of rapidly fading Type Ibc supernovae

Io Kleiser, Jim Fuller, Daniel Kasen

Type I rapidly fading supernovae (RFSNe) appear to originate from hydrogen-free stars with large radii that produce predominantly shock-cooling light curves, in contrast with more…

astro-ph.HE2018★ 140 cited

Spectra of Hydrogen-Poor Superluminous Supernovae from the Palomar Transient Factory

Robert M. Quimby, Annalisa De Cia, Avishay Gal-Yam +20

Most Type I superluminous supernovae (SLSNe-I) reported to date have been identified by their high peak luminosities and spectra lacking obvious signs of hydrogen. We demonstrate t…