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Marco Bazzan

Researcher at University of Padua

Publications -  306
Citations -  68260

Marco Bazzan is an academic researcher from University of Padua. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 83, co-authored 284 publications receiving 54421 citations. Previous affiliations of Marco Bazzan include Istituto Nazionale di Fisica Nucleare & Max Planck Society.

Papers
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Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA

B. P. Abbott, +1138 more
TL;DR: In this article, the authors present possible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves.
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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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GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$

B. P. Abbott, +1199 more
TL;DR: In 2019, the LIGO Livingston detector observed a compact binary coalescence with signal-to-noise ratio 12.9 as mentioned in this paper, which is consistent with the individual binary components being neutron stars.