68 citations · 286 across the 17 of their papers we have counts for
8 papers · 1 filter
High-precision source characterization of intermediate mass-ratio black hole coalescences with gravitational waves: The importance of higher-order multipoles
Tousif Islam, Scott E. Field, Carl-Johan Haster +1
Intermediate mass ratio inspiral (IMRI) binaries -- containing stellar-mass black holes coalescing into intermediate-mass black holes () -- are a highly anticipated…
Bayesian inference for gravitational waves from binary neutron star mergers in third-generation observatories
Rory Smith, Ssohrab Borhanian, Bangalore Sathyaprakash +10
Third-generation (3G) gravitational-wave detectors will observe thousands of coalescing neutron star binaries with unprecedented fidelity. Extracting the highest precision science…
GW190521 as a merger of Proca stars: a potential new vector boson of eV
Juan Calderón Bustillo, Nicolas Sanchis-Gual, Alejandro Torres-Forné +6
Advanced LIGO-Virgo reported a short gravitational-wave signal (GW190521) interpreted as a quasi-circular merger of black holes, one populating the pair-instability supernova gap,…
Gravitational wave detection without boot straps: a Bayesian approach
Gregory Ashton, Eric Thrane, Rory J. E. Smith
In order to separate astrophysical gravitational-wave signals from instrumental noise, which often contains transient non-Gaussian artifacts, astronomers have traditionally relied…
Massively parallel Bayesian inference for transient gravitational-wave astronomy
Rory Smith, Gregory Ashton, Avi Vajpeyi +1
Understanding the properties of transient gravitational waves and their sources is of broad interest in physics and astronomy. Bayesian inference is the standard framework for astr…
Measuring the neutron star equation of state with gravitational waves: the first forty binary neutron star mergers
Francisco Hernandez Vivanco, Rory Smith, Eric Thrane +3
Gravitational waves from binary neutron star coalescences contain rich information about matter at supranuclear densities encoded by the neutron star equation of state. We can meas…