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E. Cesarini

Researcher at University of Rome Tor Vergata

Publications -  112
Citations -  41211

E. Cesarini is an academic researcher from University of Rome Tor Vergata. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 59, co-authored 92 publications receiving 32590 citations. Previous affiliations of E. Cesarini include Istituto Nazionale di Fisica Nucleare.

Papers
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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.
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GW190412: Observation of a binary-black-hole coalescence with asymmetric masses

Richard J. Abbott, +1333 more
- 15 Aug 2020 - 
TL;DR: In this article, the authors reported the observation of gravitational waves from a binary-black-hole coalescence during the first two weeks of LIGO and Virgo's third observing run.
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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.