output
20022020
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations

Showing 2014Show all

22 papers · 1 filter

gr-qc201439 cited

The detectability of eccentric compact binary coalescences with advanced gravitational-wave detectors

Michael Coughlin, Patrick Meyers, Eric Thrane +2

Compact binary coalescences are a promising source of gravitational waves for second-generation interferometric gravitational-wave detectors such as advanced LIGO and advanced Virg…

gr-qc201455 cited

A directed search for gravitational waves from Scorpius X-1 with initial LIGO

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +891

We present results of a search for continuously-emitted gravitational radiation, directed at the brightest low-mass X-ray binary, Scorpius X-1. Our semi-coherent analysis covers 10…

gr-qc20143.5k cited

Advanced LIGO

The LIGO Scientific Collaboration

The Advanced LIGO gravitational wave detectors are second generation instruments designed and built for the two LIGO observatories in Hanford, WA and Livingston, LA. The two instru…

astro-ph.SR2014122 cited

The Binary Companion of Young, Relativistic Pulsar J1906+0746

Joeri van Leeuwen, Laura Kasian, Ingrid H. Stairs +13

PSR J1906+0746 is a young pulsar in the relativistic binary with the second-shortest known orbital period, of 3.98 hours. We here present a timing study based on five years of obse…

astro-ph.IM201450 cited

Narrow-band search of continuous gravitational-wave signals from Crab and Vela pulsars in Virgo VSR4 data

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +894

In this paper we present the results of a coherent narrow-band search for continuous gravitational-wave signals from the Crab and Vela pulsars conducted on Virgo VSR4 data. In orde…

math.AG2014

Low-dimensional factors of superelliptic Jacobians

Thomas Occhipinti, Douglas Ulmer

Given a polynomial , we consider the family of superelliptic curves and their Jacobians for varying integers . We show that for any integer $…