activity
20122022
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 · 8.2k across the 53 of their papers we have counts for

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Showing 2018Show all

10 papers · 1 filter

astro-ph.HE2018★ 4 cited

Target of Opportunity Observations of Gravitational Wave Events with LSST

R. Margutti, P. Cowperthwaite, Z. Doctor +79

The discovery of the electromagnetic counterparts to the binary neutron star merger GW170817 has opened the era of GW+EM multi-messenger astronomy. Exploiting this breakthrough req…

astro-ph.IM2018★ 31 cited

A strategy for LSST to unveil a population of kilonovae without gravitational-wave triggers

Igor Andreoni, Shreya Anand, Federica B. Bianco +10

We present a cadence optimization strategy to unveil a large population of kilonovae using optical imaging alone. These transients are generated during binary neutron star and pote…

astro-ph.IM2018★ 23 cited

Presto-Color: A Photometric Survey Cadence for Explosive Physics & Fast Transients

Federica B. Bianco, Maria R. Drout, Melissa L. Graham +6

We identify minimal observing cadence requirements that enable photometric astronomical surveys to detect and recognize fast and explosive transients and fast transient features. O…

astro-ph.HE2018★ 21 cited

A Search for Optical Emission from Binary-Black-Hole Merger GW170814 with the Dark Energy Camera

Z. Doctor, R. Kessler, K. Herner +96

Binary black hole (BBH) mergers found by the LIGO and Virgo detectors are of immense scientific interest to the astrophysics community, but are considered unlikely to be sources of…

astro-ph.HE2018★ 53 cited

LSST Target-of-Opportunity Observations of Gravitational Wave Events: Essential and Efficient

P. S. Cowperthwaite, V. A. Villar, D. M. Scolnic +1

We present simulated observations to assess the ability of LSST and the WFD survey to detect and characterize kilonovae - the optical emission associated with binary neutron star (…

astro-ph.HE2018★ 45 cited

Spitzer Space Telescope Infrared Observations of the Binary Neutron Star Merger GW170817

V. A. Villar, P. S. Cowperthwaite, E. Berger +12

We present Spitzer Space Telescope 3.6 and 4.5 micron observations of the binary neutron star merger GW170817 at 43, 74, and 264 days post-merger. Using the final observation as a…

astro-ph.HE2018★ 205 cited

A Decline in the X-ray through Radio Emission from GW170817 Continues to Support an Off-Axis Structured Jet

K. D. Alexander, R. Margutti, P. K. Blanchard +17

We present new observations of the binary neutron star merger GW170817 at days post-merger, at radio (Karl G. Jansky Very Large Array; VLA), X-ray (Chandra X-ra…

astro-ph.IM2018

Open Astronomy Catalogs API

James Guillochon, Philip S. Cowperthwaite

We announce the public release of the application program interface (API) for the Open Astronomy Catalogs (OACs), the OACAPI. The OACs serve near-complete collections of supernova,…

astro-ph.GA2018★ 152 cited

A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations

Michele Cantiello, J. B. Jensen, J. P. Blakeslee +25

The joint detection of gravitational waves and electromagnetic radiation from the binary neutron star (BNS) merger GW170817 has provided unprecedented insight into a wide range of…

astro-ph.HE2018★ 342 cited

The Binary Neutron Star event LIGO/VIRGO GW170817 a hundred and sixty days after merger: synchrotron emission across the electromagnetic spectrum

Raffaella Margutti, K. D. Alexander, X. Xie +17

We report deep Chandra, HST and VLA observations of the binary neutron star event GW170817 at d after merger. These observations show that GW170817 has been steadily bright…