activity
20182020
most citedFirst measurement of the Hubble parameter from bright binary black hole GW190521

36 citations · 36 across the 1 of their papers we have counts for

collaborators

6 papers

gr-qc2020

Gravitational wave friction in light of GW170817 and GW190521

S. Mastrogiovanni, L. Haegel, C. Karathanasis +2

We use the gravitational wave (GW) events GW170817 and GW190521, together with their proposed electromagnetic counterparts, to constrain cosmological parameters and theories of gra…

astro-ph.CO202036 cited

First measurement of the Hubble parameter from bright binary black hole GW190521

Suvodip Mukherjee, Archisman Ghosh, Matthew J. Graham +6

The Zwicky Transient Facility (ZTF) reported the event "ZTF19abanrhr" as a candidate electromagnetic (EM) counterpart at a redshift to the gravitational wave (GW) emissio…

astro-ph.HE2020

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…

astro-ph.CO2020

A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies

A. Palmese, J. deVicente, M. E. S. Pereira +85

We present a measurement of the Hubble constant using the gravitational wave (GW) event GW190814, which resulted from the coalescence of a 23 black hole with a 2.6…

gr-qc2019

Cosmological Inference using Gravitational Wave Standard Sirens: A Mock Data Challenge

Rachel Gray, Ignacio Magaña Hernandez, Hong Qi +12

The observation of binary neutron star merger GW170817, along with its optical counterpart, provided the first constraint on the Hubble constant using gravitational wave stan…

astro-ph.CO2018

A standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart

M. Fishbach, R. Gray, I. Magaña Hernandez +316

We perform a statistical standard siren analysis of GW170817. Our analysis does not utilize knowledge of NGC 4993 as the unique host galaxy of the optical counterpart to GW170817.…