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20022026
most citedLSST: from Science Drivers to Reference Design and Anticipated Data Products

3.5k citations · 10.1k across the 123 of their papers we have counts for

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7 papers · 1 filter

astro-ph.SR2026

The DESI Data Release 1 white dwarf catalogue

Andrew Swan, Boris T. Gänsicke, Paula Izquierdo +49

The Dark Energy Spectroscopic Instrument is conducting a redshift survey, mapping the universe in three dimensions to measure the history of cosmic expansion. As well as extragalac…

astro-ph.SR2015★ 200 cited

On the diversity of super-luminous supernovae: ejected mass as the dominant factor

M. Nicholl, S. J. Smartt, A. Jerkstrand +37

We assemble a sample of 24 hydrogen-poor super-luminous supernovae (SLSNe). Parameterizing the light curve shape through rise and decline timescales shows that the two are highly c…

astro-ph.SR2015★ 62 cited

SN 2009ip at late times - an interacting transient at +2 years

Morgan Fraser, Rubina Kotak, Andrea Pastorello +31

We present photometric and spectroscopic observations of the interacting transient SN 2009ip taken during the 2013 and 2014 observing seasons. We characterise the photometric evolu…

astro-ph.SR2013★ 87 cited

The supernova CSS121015:004244+132827: a clue for understanding super-luminous supernovae

S. Benetti, M. Nicholl, E. Cappellaro +24

We present optical photometry and spectra of the super luminous type II/IIn supernova CSS121015:004244+132827 (z=0.2868) spanning epochs from -30 days (rest frame) to more than 200…

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.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…