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V

V. Mangano

Researcher at Sapienza University of Rome

Publications -  223
Citations -  65547

V. Mangano is an academic researcher from Sapienza University of Rome. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 77, co-authored 189 publications receiving 51556 citations. Previous affiliations of V. Mangano include INAF & University of Glasgow.

Papers
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Journal ArticleDOI

GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run

Richard J. Abbott, +1351 more
TL;DR: In this article, the authors present 39 candidate gravitational wave events from compact binary coalescences detected by Advanced LIGO and Advanced Virgo in the first half of the third observing run (O3a) between 1 April 2019 15:00 UTC and 1 October 2019 15.00.
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Astrophysical implications of the binary black hole merger gw150914

B. P. Abbott, +964 more
TL;DR: The discovery of the GW150914 with the Advanced LIGO detectors provides the first observational evidence for the existence of binary black-hole systems that inspiral and merge within the age of the Universe as mentioned in this paper.
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Properties of the Binary Neutron Star Merger GW170817

B. P. Abbott, +1160 more
- 02 Jan 2019 - 
TL;DR: In this paper, 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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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.