activity
20142023
most citedAdvanced LIGO

3.5k citations · 6.8k across the 18 of their papers we have counts for

collaborators

18 papers

gr-qc20231 cited

DAGnabbit! Ensuring Consistency between Noise and Detection in Hierarchical Bayesian Inference

Reed Essick, Maya Fishbach

Hierarchical Bayesian inference can simultaneously account for both measurement uncertainty and selection effects within astronomical catalogs. In particular, the hierarchy imposed…

astro-ph.HE20236 cited

Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and Virgo

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1772

Despite the growing number of confident binary black hole coalescences observed through gravitational waves so far, the astrophysical origin of these binaries remains uncertain. Or…

astro-ph.EP2023

Orbital Decay of Hot Jupiters due to Weakly Nonlinear Tidal Dissipation

Nevin N. Weinberg, Niyousha Davachi, Reed Essick +3

We study tidal dissipation in hot Jupiter host stars due to the nonlinear damping of tidally driven -modes, extending the calculations of Essick & Weinberg (2016) to a wide vari…

gr-qc2023

QoQ: a Q-transform based test for Gravitational Wave transient events

Siddharth Soni, Ethan Marx, Erik Katsavounidis +6

The observation of transient gravitational waves is hindered by the presence of transient noise, colloquially referred to as glitches. These glitches can often be misidentified as…

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…

gr-qc202071 cited

All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems

The LIGO Scientific Collaboration, the Virgo Collaboration, R. Abbott +1369

Rapidly spinning neutron stars are promising sources of persistent, continuous gravitational waves. Detecting such a signal would allow probing of the physical properties of matter…