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C. Messick

13 papers hereh-index 7740.9k citations281 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author13

Across the 13 of 13 papers where every author was matched, so the position is known.

fields
  • gr-qc8
  • astro-ph.IM3
  • astro-ph.HE2
same name
  • C. Messick — 6 papers
  • C. Messick — 5 papers
  • C. Messick — 2 papers
  • C. Messick — 1 paper
  • C. Messick — 1 paper
  • C. Messick — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20242026
collaborators
Showing astro-ph.IMShow all

4 papers · 1 filter

astro-ph.IM2026

SGNL: Scalable Low-Latency Gravitational Wave Detection Pipeline for Compact Binary Mergers

Yun-Jing Huang, Chad Hanna, Leo Tsukada +8

We present SGNL, a scalable, low-latency gravitational-wave search pipeline. It reimplements the core matched-filtering principles of the GstLAL pipeline within a modernized framew…

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.IM2025

A Neural Network Approach to Preferred Event Selection for Low-Latency Gravitational-Wave Alerts

Pratyusava Baral, Cody Messick, Patrick Brady

The LIGO-Virgo-KAGRA collaboration uses multiple independent search pipelines to detect gravitational waves, often resulting in multiple triggers (g-events) for a single astrophysi…

astro-ph.IM2024

GWSkyNet II : a refined machine learning pipeline for real-time classification of public gravitational wave alerts

Man Leong Chan, Jess McIver, Ashish Mahabal +12

Electromagnetic follow-up observations of gravitational wave events offer critical insights and provide significant scientific gain from this new class of astrophysical transients.…

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