activity
20192023
most citedGROWTH on S190814bv: Deep Synoptic Limits on the Optical/Near-Infrared Counterpart to a Neutron Star-Black Hole Merger

109 citations · 440 across the 9 of their papers we have counts for

collaborators

9 papers

gr-qc2023★ 53 cited

Non-parametric inference of the population of compact binaries from gravitational wave observations using binned Gaussian processes

Anarya Ray, Ignacio Magaña Hernandez, Siddharth Mohite +2

The observation of gravitational waves from multiple compact binary coalescences by the LIGO-Virgo-KAGRA detector networks has enabled us to infer the underlying distribution of co…

astro-ph.IM2021★ 8 cited

Inferring kilonova population properties with a hierarchical Bayesian framework I : Non-detection methodology and single-event analyses

Siddharth R. Mohite, Priyadarshini Rajkumar, Shreya Anand +17

We present : a hierarchical Bayesian framework to infer the intrinsic luminosity parameters of kilonovae (KNe) associated with gravitational-wave (GW) events, based…

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.HE2020★ 79 cited

An early warning system for electromagnetic follow-up of gravitational-wave events

Surabhi Sachdev, Ryan Magee, Chad Hanna +28

Binary neutron stars (BNSs) will spend -- 15 minutes in the band of Advanced LIGO and Virgo detectors at design sensitivity. Matched-filtering of gravitational-wave (GW…

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.HE2020★ 102 cited

Kilonova Luminosity Function Constraints based on Zwicky Transient Facility Searches for 13 Neutron Star Mergers

Mansi M. Kasliwal, Shreya Anand, Tomas Ahumada +100

We present a systematic search for optical counterparts to 13 gravitational wave (GW) triggers involving at least one neutron star during LIGO/Virgo's third observing run. We searc…

astro-ph.HE2019★ 109 cited

GROWTH on S190814bv: Deep Synoptic Limits on the Optical/Near-Infrared Counterpart to a Neutron Star-Black Hole Merger

Igor Andreoni, Daniel A. Goldstein, Mansi M. Kasliwal +49

On 2019 August 14, the Advanced LIGO and Virgo interferometers detected the high-significance gravitational wave (GW) signal S190814bv. The GW data indicated that the event resulte…

astro-ph.HE2019★ 59 cited

A self-consistent method to estimate the rate of compact binary coalescences with a Poisson mixture model

Shasvath J. Kapadia, Sarah Caudill, Jolien D. E. Creighton +13

The recently published GWTC-1 - a journal article summarizing the search for gravitational waves (GWs) from coalescing compact binaries in data produced by the LIGO-Virgo network o…

gr-qc2019★ 29 cited

Sub-threshold binary neutron star search in Advanced LIGO's first observing run

Ryan Magee, Heather Fong, Sarah Caudill +12

We present a search for gravitational waves from double neutron star binaries inspirals in Advanced LIGO's first observing run. The search considers a narrow range of binary chirp…