activity
20142022
most citedGW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence

1.3k citations · 1.5k across the 7 of their papers we have counts for

collaborators

7 papers

gr-qc202216 cited

Concurrent estimation of noise and compact-binary signal parameters in gravitational-wave data

Cailin Plunkett, Sophie Hourihane, Katerina Chatziioannou

Gravitational-wave parameter estimation for compact binary signals typically relies on sequential estimation of the properties of the detector Gaussian noise and of the binary para…

astro-ph.HE202242 cited

Implicit correlations within phenomenological parametric models of the neutron star equation of state

Isaac Legred, Katerina Chatziioannou, Reed Essick +1

The rapid increase in the number and precision of astrophysical probes of neutron stars in recent years allows for the inference of their equation of state. Observations target dif…

astro-ph.HE202058 cited

You Can't Always Get What You Want: The Impact of Prior Assumptions on Interpreting GW190412

Michael Zevin, Christopher P. L. Berry, Scott Coughlin +2

GW190412 is the first observation of a black hole binary with definitively unequal masses. GW190412's mass asymmetry, along with the measured positive effective inspiral spin, allo…

astro-ph.HE20171.3k cited

GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1101

On June 8, 2017 at 02:01:16.49 UTC, a gravitational-wave signal from the merger of two stellar-mass black holes was observed by the two Advanced LIGO detectors with a network signa…

gr-qc201646 cited

Improved next-to-leading order tidal heating and torquing of a Kerr black hole

Katerina Chatziioannou, Eric Poisson, Nicolas Yunes

We calculate the energy and angular momentum fluxes across the event horizon of a tidally deformed, rapidly rotating black hole to next-to-leading order in the curvature of the ext…

gr-qc201434 cited

Toward Realistic and Practical No-Hair Relations for Neutron Stars in the Non-Relativistic Limit

Katerina Chatziioannou, Kent Yagi, Nicolas Yunes

The gravitational properties of astrophysical objects depend sensitively on their internal structure. In Newtonian theory, the gravitational potential of a rotating star can be ful…