activity
20162026
most citedKAGRA: 2.5 Generation Interferometric Gravitational Wave Detector

535 citations · 2.2k across the 67 of their papers we have counts for

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Showing astro-ph.HEShow all

5 papers · 1 filter

astro-ph.HE2025★ 2 cited

GW231109_235456: A Sub-threshold Binary Neutron Star Merger in the LIGO-Virgo-KAGRA O4a Observing Run?

Wanting Niu, Carl-Johan Haster, Jolien D. E. Creighton +25

We present a sub-threshold search for gravitational-wave inspirals from binary neutron stars using data from the first part of the fourth LIGO--Virgo--KAGRA observing run. To enhan…

astro-ph.HE2024★ 1 cited

On the association of GW190425 with its potential electromagnetic counterpart FRB 20190425A

Ignacio Magaña Hernandez, Virginia D'Emilio, Soichiro Morisaki +2

Recent work by Moroianu et al. (2022) has suggested that the binary neutron star (BNS) merger GW190425 might have a potential fast radio burst (FRB) counterpart association, FRB 20…

astro-ph.HE2023★ 30 cited

Low-latency gravitational wave alert products and their performance at the time of the fourth LIGO-Virgo-KAGRA observing run

Sushant Sharma Chaudhary, Andrew Toivonen, Gaurav Waratkar +50

Multi-messenger searches for BNS and NSBH mergers are currently one of the most exciting areas of astronomy. The search for joint electromagnetic and neutrino counterparts to GWs h…

astro-ph.HE2023★ 9 cited

Challenges for Fast Radio Bursts as Multi-Messenger Sources from Binary Neutron Star Mergers

Mohit Bhardwaj, Antonella Palmese, Ignacio Magaña Hernandez +2

Fast radio bursts (FRBs) are a newly discovered class of radio transients that emerge from cosmological sources and last for a few milliseconds. However, their origin remain…

astro-ph.HE2023★ 14 cited

Localization of binary neutron star mergers with a single Cosmic Explorer

Pratyusava Baral, Soichiro Morisaki, Ignacio Magaña Hernandez +1

Next-generation ground-based gravitational-wave detectors, such as Cosmic Explorer (CE), are expected to be sensitive to gravitational-wave signals with frequencies as low as 5 Hz,…