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most citedThe Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

1k citations · 10.3k across the 71 of their papers we have counts for

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astro-ph.HE2017★ 579 cited

The Combined Ultraviolet, Optical, and Near-Infrared Light Curves of the Kilonova Associated with the Binary Neutron Star Merger GW170817: Unified Data Set, Analytic Models, and Physical Implications

V. Ashley Villar, James Guillochon, Edo Berger +10

We present the first effort to aggregate, homogenize, and uniformly model the combined ultraviolet, optical, and near-infrared dataset for the electromagnetic counterpart of the bi…

astro-ph.HE2017★ 31 cited

Observations of SN 2015F suggest a correlation between the intrinsic luminosity of Type Ia supernovae and the shape of their light curves >900 days after explosion

Or Graur, David R. Zurek, Armin Rest +6

The late-time light curves of Type Ia supernovae (SNe Ia), observed days after explosion, present the possibility of a new diagnostic for SN Ia progenitor and explosion mode…

astro-ph.HE2017★ 1k cited

The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

P. S. Cowperthwaite, E. Berger, V. A. Villar +141

We present UV, optical, and NIR photometry of the first electromagnetic counterpart to a gravitational wave source from Advanced LIGO/Virgo, the binary neutron star merger GW170817…

astro-ph.IM2017★ 227 cited

MOSFiT: Modular Open-Source Fitter for Transients

James Guillochon, Matt Nicholl, V. Ashley Villar +5

Much of the progress made in time-domain astronomy is accomplished by relating observational multi-wavelength time series data to models derived from our understanding of physical…

astro-ph.HE2017★ 63 cited

The superluminous supernova SN 2017egm in the nearby galaxy NGC 3191: a metal-rich environment can support a typical SLSN evolution

Matt Nicholl, Edo Berger, Raffaella Margutti +4

At redshift z=0.03, the recently-discovered SN 2017egm is the nearest Type I superluminous supernova (SLSN) to date, and first near the center of a massive spiral galaxy (NGC 3191)…

astro-ph.HE2017★ 82 cited

Theoretical Models of Optical Transients. I. A Broad Exploration of the Duration-Luminosity Phase Space

V. Ashley Villar, Edo Berger, Brian D. Metzger +1

The duration-luminosity phase space of optical transients is used, mostly heuristically, to compare various classes of transient events, to explore the origin of new transients, an…