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B. L. Pearlstone

Researcher at University of Glasgow

Publications -  136
Citations -  55060

B. L. Pearlstone is an academic researcher from University of Glasgow. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 72, co-authored 136 publications receiving 44830 citations.

Papers
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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, +1138 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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GW150914: The Advanced LIGO Detectors in the Era of First Discoveries

B. P. Abbott, +958 more
TL;DR: Following a major upgrade, the two advanced detectors of the Laser Interferometer Gravitational-wave Observatory (LIGO) held their first observation run between September 2015 and January 2016, and observed a transient gravitational-wave signal determined to be the coalescence of two black holes.
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Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA

B. P. Abbott, +1318 more
TL;DR: In this paper, the authors present the current best estimate of the plausible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA detectors over the next several years, with the intention of providing information to facilitate planning for multi-messenger astronomy with gravitational waves.
Journal ArticleDOI

Properties of the binary neutron star merger GW170817

B. P. Abbott, +1146 more
TL;DR: In this article, the authors improved initial estimates of the binary's properties, including component masses, spins, and tidal parameters, using the known source location, improved modeling, and recalibrated Virgo data.
Journal ArticleDOI

Tests of general relativity with the binary black hole signals from the LIGO-Virgo catalog GWTC-1

B. P. Abbott, +1141 more
- 20 Nov 2019 - 
TL;DR: In this paper, the authors present four tests of the consistency of the data with binary black hole gravitational waveforms predicted by general relativity, including the best-fit waveform from the data and the consistency with detector noise.