activity
20182025
most citedBayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue

503 citations · 1.5k across the 19 of their papers we have counts for

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5 papers · 1 filter

astro-ph.HE2025★ 10 cited

Kilonova constraints for the LIGO/Virgo/KAGRA neutron star merger candidate S250206dm: GW-MMADS observations

Lei Hu, Tomás Cabrera, Antonella Palmese +35

Gravitational wave (GW) neutron star mergers with an associated electromagnetic counterpart constitute powerful probes of binary evolution, the production sites of heavy elements,…

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,…

astro-ph.HE2021★ 2 cited

Constraining the number of spacetime dimensions from GWTC-3 binary black hole mergers

Ignacio Magana Hernandez

In modified gravity models that allow for additional non-compact spacetime dimensions, energy from gravitational waves can leak into these extra spacetime dimensions, leading to a…

astro-ph.HE2020★ 83 cited

Current observations are insufficient to confidently associate the binary black hole merger GW190521 with AGN J124942.3+344929

Gregory Ashton, Kendall Ackley, Ignacio Magaña Hernandez +1

Recently, Graham et al. (2020) identified ZTF19abanrhr as a candidate electromagnetic counterpart to the binary black hole merger GW190521. The authors argue that the observations…

astro-ph.HE2020★ 86 cited

Identifying strong gravitational-wave lensing during the second observing run of Advanced LIGO and Advanced Virgo

Xiaoshu Liu, Ignacio Magana Hernandez, Jolien Creighton

We perform Bayesian model selection with parameter estimation to identify potentially lensed gravitational-wave images from the second observing run (O2) of Advanced LIGO and Advan…