activity
20152020
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 · 6.1k across the 24 of their papers we have counts for

collaborators

42 papers

astro-ph.CO202071 cited

A Program for Multi-Messenger Standard Siren Cosmology in the Era of LIGO A+, Rubin Observatory, and Beyond

Hsin-Yu Chen, Philip S. Cowperthwaite, Brian D. Metzger +1

The most promising variation of the standard siren technique combines gravitational-wave (GW) data for binary neutron star (BNS) mergers with redshift measurements enabled by their…

astro-ph.HE2020

The Rise and Fall of ASASSN-18pg: Following a TDE from Early To Late Times

Thomas W. -S. Holoien, Katie Auchettl, Michael A. Tucker +29

We present nearly 500 days of observations of the tidal disruption event ASASSN-18pg, spanning from 54 days before peak light to 441 days after peak light. Our dataset includes X-r…

astro-ph.HE2020

The Tidal Disruption Event AT 2018hyz II: Light Curve Modeling of a Partially Disrupted Star

Sebastian Gomez, Matt Nicholl, Philip Short +18

AT 2018hyz (=ASASSN-18zj) is a tidal disruption event (TDE) located in the nucleus of a quiescent E+A galaxy at a redshift of , first detected by the All-Sky Automated…

astro-ph.IM2020

Optical follow-up of gravitational wave triggers with DECam during the first two LIGO/VIRGO observing runs

K. Herner, J. Annis, D. Brout +82

Gravitational wave (GW) events detectable by LIGO and Virgo have several possible progenitors, including black hole mergers, neutron star mergers, black hole--neutron star mergers,…

gr-qc201985 cited

Enabling real-time multi-messenger astrophysics discoveries with deep learning

E. A. Huerta, Gabrielle Allen, Igor Andreoni +57

Multi-messenger astrophysics is a fast-growing, interdisciplinary field that combines data, which vary in volume and speed of data processing, from many different instruments that…

astro-ph.HE2019

Two years of non-thermal emission from the binary neutron star merger GW170817: rapid fading of the jet afterglow and first constraints on the kilonova fastest ejecta

A. Hajela, R. Margutti, K. D. Alexander +27

We present Chandra and VLA observations of GW170817 at ~521-743 days post merger, and a homogeneous analysis of the entire Chandra data set. We find that the late-time non-thermal…