activity
20102026
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 10.6k across the 186 of their papers we have counts for

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Showing astro-ph.COShow all

9 papers · 1 filter

astro-ph.CO2020★ 26 cited

The first Hubble diagram and cosmological constraints using superluminous supernova

C. Inserra, M. Sullivan, C. R. Angus +88

We present the first Hubble diagram of superluminous supernovae (SLSNe) out to a redshift of two, together with constraints on the matter density, , and the dark energy…

astro-ph.CO2017★ 32 cited

Euclid: Superluminous supernovae in the Deep Survey

C. Inserra, R. C. Nichol, D. Scovacricchi +31

In the last decade, astronomers have found a new type of supernova called `superluminous supernovae' (SLSNe) due to their high peak luminosity and long light-curves. These hydrogen…

astro-ph.CO2013★ 74 cited

The superluminous supernova PS1-11ap: bridging the gap between low and high redshift

M. McCrum, S. J. Smartt, R. Kotak +37

We present optical photometric and spectroscopic coverage of the superluminous supernova (SLSN) PS1-11ap, discovered with the Pan-STARRS1 Medium Deep Survey at z = 0.524. This intr…

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★ 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…