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20072026
most citedThe Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart

584 citations · 1.5k across the 31 of their papers we have counts for

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11 papers · 1 filter

astro-ph.IM2026

Method to get Better Sky Maps in a GstLAL Low-Latency Analysis

Prathamesh Joshi, Becca Ewing, Chad Hanna +40

Modeled gravitational wave searches correlate the strain data with a bank of gravitational wave template waveforms to make detections of gravitational wave candidates, and these re…

astro-ph.IM2023★ 53 cited

Improved ranking statistics of the GstLAL inspiral search for compact binary coalescences

Leo Tsukada, Prathamesh Joshi, Shomik Adhicary +37

Starting from May 2023, the LIGO Scientific, Virgo and KAGRA Collaboration is planning to conduct the fourth observing run with improved detector sensitivities and an expanded dete…

astro-ph.IM2020

Automating the Inclusion of Subthreshold Signal-to-Noise Ratios for Rapid Gravitational-Wave Localization

Cody Messick, Surabhi Sachdev, Kipp Cannon +29

The accurate localization of gravitational-wave (GW) events in low-latency is a crucial element in the search for further multimessenger signals from these cataclysmic events. The…

astro-ph.IM2020

GstLAL: A software framework for gravitational wave discovery

Kipp Cannon, Sarah Caudill, Chiwai Chan +28

The GstLAL library, derived from Gstreamer and the LIGO Algorithm Library, supports a stream-based approach to gravitational-wave data processing. Although GstLAL was primarily des…

astro-ph.IM2020★ 1 cited

Improving the background estimation technique in the GstLAL inspiral pipeline with the time-reversed template bank

Chiwai Chan, Kipp Cannon, Sarah Caudill +20

Background estimation is important for determining the statistical significance of a gravitational-wave event. Currently, the background model is constructed numerically from the s…

astro-ph.IM2020★ 2 cited

iDQ: Statistical Inference of Non-Gaussian Noise with Auxiliary Degrees of Freedom in Gravitational-Wave Detectors

Reed Essick, Patrick Godwin, Chad Hanna +2

Gravitational-wave detectors are exquisitely sensitive instruments and routinely enable ground-breaking observations of novel astronomical phenomena. However, they also witness non…

astro-ph.IM2019★ 2 cited

Cyberinfrastructure Requirements to Enhance Multi-messenger Astrophysics

Philip Chang, Gabrielle Allen, Warren Anderson +39

The identification of the electromagnetic counterpart of the gravitational wave event, GW170817, and discovery of neutrinos and gamma-rays from TXS 0506+056 heralded the new era of…

astro-ph.IM2018★ 34 cited

Methods for the detection of gravitational waves from sub-solar mass ultracompact binaries

Ryan Magee, Anne-Sylvie Deutsch, Phoebe McClincy +6

We describe detection methods for extensions of gravitational wave searches to sub-solar mass compact binaries. Sub-solar mass searches were previously carried out using Initial LI…

astro-ph.IM2018★ 7 cited

Multi-Messenger Astrophysics: Harnessing the Data Revolution

Gabrielle Allen, Warren Anderson, Erik Blaufuss +27

The past year has witnessed discovery of the first identified counterparts to a gravitational wave transient (GW 170817A) and a very high-energy neutrino (IceCube-170922A). These s…

astro-ph.IM2017★ 35 cited

Systematic errors in estimation of gravitational-wave candidate significance

Collin Capano, Thomas Dent, Chad Hanna +4

The statistical significance of a candidate gravitational-wave (GW) event is crucial to the prospects for a confirmed detection, or for its selection as a candidate for follow-up e…

astro-ph.IM2015★ 8 cited

Likelihood-Ratio Ranking Statistic for Compact Binary Coalescence Candidates with Rate Estimation

Kipp Cannon, Chad Hanna, Jacob Peoples

We present a new likelihood-ratio ranking statistic for use in searches for gravitational waves from the inspiral and merger of compact object binaries. Expanding on previous work,…