Web application for galaxy-targeted follow-up of electromagnetic counterparts to gravitational wave sources
L. Salmon, L. Hanlon, R. M. Jeffrey, A. Martin-Carrillo

TL;DR
This paper introduces a publicly accessible web tool that rapidly identifies and ranks galaxies for follow-up observations of gravitational wave events, aiding multi-messenger astronomy efforts.
Contribution
It presents a new web interface with a fast galaxy retrieval algorithm that scores and ranks galaxies based on gravitational wave data, improving follow-up efficiency.
Findings
Algorithm retrieves and ranks galaxies within minutes
Web application tested on past events with successful performance
Automated triggering during observing runs enhances follow-up speed
Abstract
The Laser Interferometer Gravitational Wave Observatory (LIGO) and Virgo Collaboration's Observing Run 3 has demanded the development of widely-applicable tools for gravitational wave follow-up. These tools must address the main challenges of the multi-messenger era, namely covering large localisation regions and quickly identifying decaying transients. To address these challenges, we present a public web interface to assist astronomers in conducting galaxy-targeted follow-up of gravitational wave events by offering a fast and public list of targets post-gravitational wave trigger. After a gravitational wave trigger, the back-end galaxy retrieval algorithm identifies and scores galaxies based on the LIGO and Virgo computed probabilities and properties of the galaxies taken from the Galaxy List for the Advanced Detector Era (GLADE) V2 galaxy catalogue. Within minutes, the user can…
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