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Yuri Levin

Researcher at Columbia University

Publications -  29
Citations -  1928

Yuri Levin is an academic researcher from Columbia University. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 20, co-authored 29 publications receiving 1592 citations. Previous affiliations of Yuri Levin include Monash University, Clayton campus & York University.

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Journal ArticleDOI

Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo

B. P. Abbott, +1218 more
TL;DR: In this paper, the mass, spin, and redshift distributions of binary black hole (BBH) mergers with LIGO and Advanced Virgo observations were analyzed using phenomenological population models.
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A guide to LIGO–Virgo detector noise and extraction of transient gravitational-wave signals

B. P. Abbott, +1165 more
TL;DR: The LIGO Scientific Collaboration and the Virgo Collaboration have cataloged eleven confidently detected gravitational-wave events during the first two observing runs of the advanced detector era as discussed by the authors.
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First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary-Black-hole Merger GW170814

Marcelle Soares-Santos, +1288 more
TL;DR: In this article, a multi-messenger measurement of the Hubble constant H 0 using the binary-black-hole merger GW170814 as a standard siren, combined with a photometric redshift catalog from the Dark Energy Survey (DES), is presented.
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All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

B. P. Abbott, +1225 more
- 08 Jul 2019 - 
TL;DR: In this article, the results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast spinning neutron stars with an asymmetry around their rotation axis, were presented.
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Precessing flaring magnetar as a source of repeating FRB 180916.J0158+65

TL;DR: In this article, it was shown that the fast radio bursts are created by giant magnetic flares of a hyper-active magnetar driven by fast ambipolar diffusion in the core, and the resulting torques and displacements of the principal axes of inertia are capable of pumping a significant amplitude of precession.