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20092026
most citedImproved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples

1.9k citations · 13.9k across the 74 of their papers we have counts for

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Showing 2015Show all

8 papers · 1 filter

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…

astro-ph.HE2015★ 94 cited

Type II supernova energetics and comparison of light curves to shock-cooling models

Adam Rubin, Avishay Gal-Yam, Annalisa De Cia +37

During the first few days after explosion, Type II supernovae (SNe) are dominated by relatively simple physics. Theoretical predictions regarding early-time SN light curves in the…

astro-ph.HE2015★ 27 cited

Supernova 2013fc in a circumnuclear ring of a luminous infrared galaxy: the big brother of SN 1998S

T. Kangas, S. Mattila, E. Kankare +30

We present photometric and spectroscopic observations of SN 2013fc, a bright type II supernova (SN) in a circumnuclear star-forming ring in the luminous infrared galaxy ESO 154-G01…

astro-ph.CO2015★ 152 cited

Rapidly Rising Transients in the Supernova - Superluminous Supernova Gap

Iair Arcavi, William M. Wolf, D. Andrew Howell +26

We present observations of four rapidly rising (t_{rise}~10d) transients with peak luminosities between those of supernovae (SNe) and superluminous SNe (M_{peak}~-20) - one discove…

astro-ph.SR2015★ 49 cited

On type IIn/Ia-CSM supernovae as exemplified by SN 2012ca

C. Inserra, M. Fraser, S. J. Smartt +15

We present the complete set of ultra-violet, optical and near-infrared photometry and spectroscopy for SN 2012ca, covering the period from 6~days prior to maximum light, until 531…

astro-ph.SR2015★ 12 cited

Spectral Models for Early Time SN 2011fe Observations

E. Baron, P. Hoeflich Brian Friesen, M. Sullivan +11

We use observed UV through near IR spectra to examine whether SN 2011fe can be understood in the framework of Branch-normal SNe Ia and to examine its individual peculiarities. As a…