activity
20162019
most citedThe Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. VII. Properties of the Host Galaxy and Constraints on the Merger Timescale

143 citations · 304 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.GA201983 cited

Beyond UVJ: More Efficient Selection of Quiescent Galaxies With UV / Mid-IR Fluxes

Joel Leja, Sandro Tacchella, Charlie Conroy

The UVJ color-color diagram is a popular and efficient method to distinguish between quiescent and star-forming galaxies through their rest-frame vs. colors. Here we ex…

astro-ph.HE201915 cited

Measuring the delay time distribution of binary neutron stars. III. Using the individual star formation histories of gravitational wave event host galaxies in the local universe

Mohammadtaher Safarzadeh, Edo Berger, Joel Leja +1

In Paper I (Safarzadeh & Berger 2019) we studied the determination of the delay time distribution (DTD) of binary neutron stars (BNS) through scaling relations between halo/stellar…

astro-ph.HE2017143 cited

The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. VII. Properties of the Host Galaxy and Constraints on the Merger Timescale

P. K. Blanchard, E. Berger, W. Fong +21

We present the properties of NGC 4993, the host galaxy of GW170817, the first gravitational wave (GW) event from the merger of a binary neutron star (BNS) system and the first with…

astro-ph.HE201763 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.GA2016

Evidence for non-stellar rest-frame near-IR emission associated with increased star formation in galaxies at

Johannes U. Lange, Pieter G. van Dokkum, Ivelina G. Momcheva +5

We explore the presence of non-stellar rest-frame near-IR () emission in galaxies at . Previous studies identified this excess in relatively small samp…