activity
20042026
most citedGW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence

2.2k citations · 8.6k across the 68 of their papers we have counts for

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11 papers · 1 filter

astro-ph.IM2026

MARVEL: A Multi Agent-based Research Validator and Enabler using Large Language Models

Nikhil Mukund, Yifang Luo, Fan Zhang +2

We present MARVEL (https://ligogpt.mit.edu/marvel), a locally deployable, open-source framework for domain-aware question answering and assisted scientific research. It is designed…

astro-ph.IM2025

GW-YOLO: Multi-transient segmentation in LIGO using computer vision

Siddharth Soni, Nikhil Mukund, Erik Katsavounidis

Time series data and their time-frequency representations from gravitational-wave interferometers present opportunities for artificial intelligence methods in signal and image proc…

astro-ph.IM2025

A machine learning-enabled search for binary black hole mergers in LIGO-Virgo-KAGRAs third observing run

Ethan Marx, William Benoit, Trevor Blodgett +8

We conduct a search for stellar-mass binary black hole mergers in gravitational-wave data collected by the LIGO detectors during the LIGO-Virgo-KAGRA (LVK) third observing run (O3)…

astro-ph.IM2024★ 1 cited

Kilonova Light Curve Parameter Estimation Using Likelihood-Free Inference

Malina Desai, Deep Chatterjee, Sahil Jhawar +3

Rapid parameter estimation is critical when dealing with short lived signals such as kilonovae. We present a parameter estimation algorithm that combines likelihood-free inference…

astro-ph.IM2023

GWAK: Gravitational-Wave Anomalous Knowledge with Recurrent Autoencoders

Ryan Raikman, Eric A. Moreno, Ekaterina Govorkova +10

Matched-filtering detection techniques for gravitational-wave (GW) signals in ground-based interferometers rely on having well-modeled templates of the GW emission. Such techniques…

astro-ph.IM2021★ 233 cited

LIGO Detector Characterization in the Second and Third Observing Runs

D. Davis, J. S. Areeda, B. K. Berger +284

The characterization of the Advanced LIGO detectors in the second and third observing runs has increased the sensitivity of the instruments, allowing for a higher number of detecta…