activity
20062023
most citedSkyMapper Southern Survey: First Data Release (DR1)

397 citations · 3.7k across the 41 of their papers we have counts for

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Showing 2013Show all

7 papers · 1 filter

astro-ph.CO2013★ 198 cited

The first month of evolution of the slow rising type II-P SN 2013ej in M74

S. Valenti, D. Sand, A. Pastorello +14

We present early photometric and spectroscopic observations of SN 2013ej, a bright type IIP supernova in M74. SN 2013ej is one of the closest SNe ever discovered. The available arc…

astro-ph.CO2013★ 71 cited

On the progenitor of the Type IIP SN 2013ej in M74

Morgan Fraser, Justyn R. Maund, Stephen J. Smartt +10

We use natural seeing imaging of SN 2013ej in M74 to identify a progenitor candidate in archival {\it Hubble Space Telescope} + ACS images. We find a source coincident with the SN…

astro-ph.CO2013★ 39 cited

Locations of Peculiar Supernovae as a Diagnostic of Their Origins

Fang Yuan, Chiaki Kobayashi, Brian P. Schmidt +3

We put constraints on the properties of the progenitors of peculiar calcium-rich transients using the distribution of locations within their host galaxies. We confirm that this cla…

astro-ph.SR2013★ 137 cited

SN 2009ip á la PESSTO: No evidence for core-collapse yet

Morgan Fraser, Cosimo Inserra, Anders Jerkstrand +35

We present observations of the interacting transient SN 2009ip, from the start of the outburst in October 2012 until the end of the 2012 observing season. The transient reached a p…

astro-ph.CO2013★ 182 cited

Rates of Superluminous Supernovae at z~0.2

Robert M. Quimby, Fang Yuan, Car Akerlof +1

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 litera…

astro-ph.SR2013★ 71 cited

PESSTO monitoring of SN 2012hn: further heterogeneity among faint type I supernovae

S. Valenti, F. Yuan, S. Taubenberger +24

We present optical and infrared monitoring data of SN 2012hn collected by the Public ESO Spectroscopic Survey for Transient Objects (PESSTO). We show that SN 2012hn has a faint pea…