activity
20062018
most citedCOSMOS Photometric Redshifts with 30-bands for 2-deg2

1.2k citations · 9.8k across the 54 of their papers we have counts for

collaborators

54 papers

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…

astro-ph.HE2016★ 29 cited

SN 2012aa - a transient between Type Ibc core-collapse and superluminous supernovae

R. Roy, J. Sollerman, J. M. Silverman +21

Context: Research on supernovae (SNe) over the past decade has confirmed that there is a distinct class of events which are much more luminous (by mag) than canonical core-…

astro-ph.CO2016★ 22 cited

Light Curves of 213 Type Ia Supernovae from the ESSENCE Survey

Gautham Narayan, Armin Rest, Brad E. Tucker +34

The ESSENCE survey discovered 213 Type Ia supernovae at redshifts 0.1 < z < 0.81 between 2002 and 2008. We present their R and I-band photometry, measured from images obtained usin…

astro-ph.HE2016★ 24 cited

Metallicity from Type II Supernovae from the (i)PTF

F. Taddia, P. Moquist, J. Sollerman +13

Type IIP supernovae (SNe IIP) have recently been proposed as metallicity () probes. The spectral models of Dessart et al. (2014) showed that the pseudo-equivalent width of Fe II…

astro-ph.HE2016★ 55 cited

Long-rising Type II supernovae from PTF and CCCP

F. Taddia, J. Sollerman, C. Fremling +17

Supernova (SN) 1987A was a peculiar H-rich event with a long-rising (LR) light curve (LC), stemming from a compact blue supergiant star (BSG). Only a few similar events have been p…

astro-ph.HE2015★ 246 cited

Flash Spectroscopy: Emission Lines from the Ionized Circumstellar Material around -Day-Old Type II Supernovae

D. Khazov, O. Yaron, A. Gal-Yam +24

Supernovae (SNe) embedded in dense circumstellar material (CSM) may show prominent emission lines in their early-time spectra ( days after the explosion), owing to recombi…