activity
20082026
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 6.2k across the 231 of their papers we have counts for

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Showing 2017Show all

5 papers · 1 filter

astro-ph.SR2017★ 36 cited

Accretion signatures in the X-shooter spectrum of the substellar companion to SR12

Alejandro Santamaría-Miranda, Claudio Cáceres, Matthias R. Schreiber +5

About a dozen substellar companions orbiting young stellar objects or pre-main sequence stars at several hundred au have been identified in the last decade. These objects are inter…

astro-ph.HE2017★ 888 cited

A kilonova as the electromagnetic counterpart to a gravitational-wave source

S. J. Smartt, T. -W. Chen, A. Jerkstrand +118

Gravitational waves were discovered with the detection of binary black hole mergers and they should also be detectable from lower mass neutron star mergers. These are predicted to…

astro-ph.HE2017★ 57 cited

A comparison between SALT/SAAO observations and kilonova models for AT 2017gfo: the first electromagnetic counterpart of a gravitational wave transient - GW170817

David A. H. Buckley, Igor Andreoni, Sudhanshu Barway +13

We report on SALT low resolution optical spectroscopy and optical/IR photometry undertaken with other SAAO telescopes (MASTER-SAAO and IRSF) of the kilonova AT 2017gfo (aka SSS17a)…

astro-ph.HE2017★ 152 cited

The Rapid Reddening and Featureless Optical Spectra of the optical counterpart of GW170817, AT 2017gfo, During the First Four Days

Curtis McCully, Daichi Hiramatsu, D. Andrew Howell +17

We present the spectroscopic evolution of AT 2017gfo, the optical counterpart of the first binary neutron star (BNS) merger detected by LIGO and Virgo, GW170817. While models have…

astro-ph.GA2017★ 20 cited

The Structure of the Young Star Cluster NGC 6231. II. Structure, Formation, and Fate

Michael A. Kuhn, Konstantin V. Getman, Eric D. Feigelson +5

The young cluster NGC 6231 (stellar ages ~2-7 Myr) is observed shortly after star-formation activity has ceased. Using the catalog of 2148 probable cluster members obtained from Ch…