papers

Publications (27)

physics.ins-det2021

Point absorbers in Advanced LIGO

Aidan F. Brooks, Gabriele Vajente, Hiro Yamamoto +198

Small, highly absorbing points are randomly present on the surfaces of the main interferometer optics in Advanced LIGO. The resulting nano-meter scale thermo-elastic deformations a…

gr-qc2018

PyCBC Live: Rapid Detection of Gravitational Waves from Compact Binary Mergers

Alexander H. Nitz, Tito Dal Canton, Derek Davis +1

We introduce an efficient and straightforward technique for rapidly detecting gravitational waves from compact binary mergers. We show that this method achieves the low latencies r…

astro-ph.IM2023

Identifying glitches near gravitational-wave signals from compact binary coalescences using the Q-transform

Leah Vazsonyi, Derek Davis

We present a computational method to identify glitches in gravitational-wave data that occur nearby gravitational-wave signals from compact binary coalescences. The Q-transform, an…

gr-qc2023

pygwb: Python-based library for gravitational-wave background searches

Arianna I. Renzini, Alba Romero-Rodrguez, Colm Talbot +31

The collection of gravitational waves (GWs) that are either too weak or too numerous to be individually resolved is commonly referred to as the gravitational-wave background (GWB).…

astro-ph.HE2022

Impact of noise transients on low latency gravitational-wave event localisation

Ronaldas Macas, Joshua Pooley, Laura K. Nuttall +6

Gravitational-wave (GW) data contains non-Gaussian noise transients called "glitches". During the third LIGO-Virgo observing run about 24% of all gravitational-wave candidates were…

gr-qc2025

The anti-aligned spin of GW191109: glitch mitigation and its implications

Rhiannon Udall, Sophie Hourihane, Simona Miller +4

With a high total mass and an inferred effective spin anti-aligned with the orbital axis at the 99.9% level, GW191109 is one of the most promising candidates for a dynamical format…

astro-ph.HE2024

An Optically Targeted Search for Gravitational Waves emitted by Core-Collapse Supernovae during the Third Observing Run of Advanced LIGO and Advanced Virgo

Marek J. Szczepańczyk, Yanyan Zheng, Javier M. Antelis +35

We present the results from a search for gravitational-wave transients associated with core-collapse supernovae observed optically within 30 Mpc during the third observing run of A…

astro-ph.IM2022

Mitigating the effects of instrumental artifacts on source localizations

Maggie C. Huber, Derek Davis

Instrumental artifacts in gravitational-wave strain data can overlap with gravitational-wave detections and significantly impair the accuracy of the measured source localizations.…

gr-qc2022

The curious case of GW200129: interplay between spin-precession inference and data-quality issues

Ethan Payne, Sophie Hourihane, Jacob Golomb +3

Measurement of spin-precession in black hole binary mergers observed with gravitational waves is an exciting milestone as it relates to both general relativistic dynamics and astro…

gr-qc2024

Gravity Spy: Lessons Learned and a Path Forward

Michael Zevin, Corey B. Jackson, Zoheyr Doctor +23

The Gravity Spy project aims to uncover the origins of glitches, transient bursts of noise that hamper analysis of gravitational-wave data. By using both the work of citizen-scienc…

astro-ph.IM2022

Bayesian modelling of scattered light in the LIGO interferometers

Rhiannon Udall, Derek Davis

Excess noise from scattered light poses a persistent challenge in the analysis of data from gravitational wave detectors such as LIGO. We integrate a physically motivated model for…

gr-qc2022

Accurate modeling and mitigation of overlapping signals and glitches in gravitational-wave data

Sophie Hourihane, Katerina Chatziioannou, Marcella Wijngaarden +3

The increasing sensitivity of gravitational-wave detectors has brought about an increase in the rate of astrophysical signal detections as well as the rate of "glitches"; transient…

physics.ins-det2019

Blip glitches in Advanced LIGO data

Miriam Cabero, Andrew Lundgren, Alex H. Nitz +8

Blip glitches are short noise transients present in data from ground-based gravitational-wave observatories. These glitches resemble the gravitational-wave signature of massive bin…

gr-qc2026

Joint inference for gravitational-wave signal and noise glitch: Method and application

Shun Yin Cheung, Rhiannon Udall, Derek Davis +2

Non-Gaussian noise transients ("glitches") in gravitational-wave observatories degrade our ability to accurately perform astrophysical inference. We present the analysis pipeline b…

gr-qc2026

Coalescing Compact Binary Parameter Estimation with Gravitational Waves in the Presence of non-Gaussian Transient Noise

Yannick Lecoeuche, Jess McIver, Alan M. Knee +7

Data from gravitational-wave (GW) detectors often contains a high rate of non-Gaussian transient noise, known as glitches. The parameters estimated from GW signals coinciding with…

gr-qc2023

General-relativistic precession in a black-hole binary

Mark Hannam, Charlie Hoy, Jonathan E. Thompson +24

The general-relativistic phenomenon of spin-induced orbital precession has not yet been observed in strong-field gravity. Gravitational-wave observations of binary black holes (BBH…

astro-ph.HE2025

Low-latency Forecasts of Kilonova Light Curves for Rubin and ZTF

Natalya Plestkova, Niharika Sravan, R. Weizmann Kiendrebeogo +11

Follow-up of gravitational-wave events by wide-field surveys is a crucial tool for the discovery of electromagnetic counterparts to gravitational wave sources, such as kilonovae. M…

gr-qc2026

Inferring the spins of merging black holes in the presence of data-quality issues

Rhiannon Udall, Sophie Bini, Katerina Chatziioannou +5

Gravitational waves from black hole binary mergers carry information about the component spins, but inference is sensitive to analysis assumptions, which may be broken by terrestri…

gr-qc2022

Incorporating information from LIGO data quality streams into the PyCBC search for gravitational waves

Derek Davis, Max Trevor, Simone Mozzon +1

We present a new method which accounts for changes in the properties of gravitational-wave detector noise over time in the PyCBC search for gravitational waves from compact binary…

astro-ph.IM2026

Rapid data quality investigations of gravitational-wave events with the Data Quality Report Builder toolkit

Derek Davis, Zach Yarbrough, Joseph Areeda +30

We present the Data Quality Report Builder toolkit, DQRbuild, a suite of data quality tools that have been developed to vet gravitational-wave events in preparation for the fourth…

gr-qc2022

Science-Driven Tunable Design of Cosmic Explorer Detectors

Varun Srivastava, Derek Davis, Kevin Kuns +6

Ground-based gravitational-wave detectors like Cosmic Explorer can be tuned to improve their sensitivity at high or low frequencies by tuning the response of the signal extraction…

gr-qc2020

Utilizing aLIGO Glitch Classifications to Validate Gravitational-Wave Candidates

Derek Davis, Laurel V. White, Peter R. Saulson

Advanced LIGO data contains numerous noise transients, or "glitches", that have been shown to reduce the sensitivity of matched filter searches for gravitational waves from compact…

astro-ph.IM2026

OmegaNeuron: Applying GravitySpy Similarity Methods to the Search for LIGO Glitch Witnesses

Bri Aleman, Derek Davis

Gravitational-wave (GW) astronomy has advanced our understanding of compact mergers through instruments like the Laser Interferometer Gravitational-Wave Observatory (LIGO). However…

gr-qc2025

Phase consistency test to identify type II strongly lensed gravitational wave signals using a single event

Kelsie Taylor, Derek Davis, Rico K. L. Lo

For gravitationally lensed type II signals, the phase of the dominant (2, 2) mode and the higher order (3, 3) mode is offset by , or roughly -0.26 radians. Using this, we d…

gr-qc2024

A new method to distinguish gravitational-wave signals from detector noise transients with Gravity Spy

Seraphim Jarov, Sarah Thiele, Siddharth Soni +5

The Advanced LIGO and Advanced Virgo detectors have enabled the confident detection of dozens of mergers of black holes and neutron stars. However, the presence of detector noise t…

astro-ph.IM2025

Guiding interferometer improvements with the frequency-dependent inspiral range

Derek Davis, Elenna Capote

The inspiral range is the most common metric for characterizing the performance of ground-based gravitational-wave interferometers. However, there is no clear formalism for working…

astro-ph.IM2024

Technical Noise, Data Quality, and Calibration Requirements for Next-Generation Gravitational-Wave Science

Elenna Capote, Louis Dartez, Derek Davis

The next generation of ground-based gravitational-wave interferometers is expected to generate a bounty of new astrophysical discoveries, with sensitivities and bandwidths greatly…