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T

T. Sadecki

Researcher at National Science Foundation

Publications -  166
Citations -  55022

T. Sadecki is an academic researcher from National Science Foundation. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 71, co-authored 156 publications receiving 43516 citations.

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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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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.
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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.
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Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog

Richard J. Abbott, +1431 more
TL;DR: In this article, the population of 47 compact binary mergers detected with a false-alarm rate of 0.614 were dynamically assembled, and the authors found that the BBH rate likely increases with redshift, but not faster than the star formation rate.