activity
20092023
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 10.3k across the 123 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

6 papers · 1 filter

astro-ph.CO2013★ 272 cited

Slowly fading super-luminous supernovae that are not pair-instability explosions

M. Nicholl, S. J. Smartt, A. Jerkstrand +57

Super-luminous supernovae that radiate more than 10^44 ergs per second at their peak luminosity have recently been discovered in faint galaxies at redshifts of 0.1-4. Some evolve s…

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★ 62 cited

PS1-12sk is a Peculiar Supernova From a He-rich Progenitor System in a Brightest Cluster Galaxy Environment

N. E. Sanders, A. M. Soderberg, R. J. Foley +29

We report on our discovery and observations of the Pan-STARRS1 supernova (SN) PS1-12sk, a transient with properties that indicate atypical star formation in its host galaxy cluster…

astro-ph.CO2012★ 84 cited

The host galaxy of the super-luminous SN 2010gx and limits on explosive nickel-56 production

Ting-Wan Chen, Stephen J. Smartt, Fabio Bresolin +6

Super-luminous supernovae have a tendency to occur in faint host galaxies which are likely to have low mass and low metallicity. While these extremely luminous explosions have been…

astro-ph.CO2012★ 25 cited

Supernovae and radio transients in M 82

S. Mattila, M. Fraser, S. J. Smartt +4

We present optical and near-infrared (IR) photometry and near-IR spectroscopy of SN 2004am, the only optically detected supernova (SN) in M 82. These demonstrate that SN 2004am was…

astro-ph.CO2009★ 89 cited

On the progenitor and early evolution of the type II supernova 2009kr

M. Fraser, K. Takats, A. Pastorello +13

We report the identification of a source coincident with SN 2009kr in HST pre-explosion images. The object appears to be a single point source with an intrinsic colour V-I = 1.1 an…