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D. D. White

Researcher at California State University, Fullerton

Publications -  23
Citations -  7408

D. D. White is an academic researcher from California State University, Fullerton. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 8, co-authored 22 publications receiving 6192 citations. Previous affiliations of D. D. White include University of California, Davis.

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The CMS experiment at the CERN LHC

S. Chatrchyan, +3175 more
TL;DR: The Compact Muon Solenoid (CMS) detector at the Large Hadron Collider (LHC) at CERN as mentioned in this paper was designed to study proton-proton (and lead-lead) collisions at a centre-of-mass energy of 14 TeV (5.5 TeV nucleon-nucleon) and at luminosities up to 10(34)cm(-2)s(-1)
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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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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.
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Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog

Richard J. Abbott, +1337 more
TL;DR: In this article, the population of the 47 compact binary mergers detected with a false-alarm rate 1/yr in the second LIGO-Virgo Gravitational-Wave Transient Catalog, GWTC-2.
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LIGO Detector Characterization in the Second and Third Observing Runs

D. Davis, +303 more
TL;DR: The characterization of the Advanced LIGO detectors in the second and third observing runs has increased the sensitivity of the instruments, allowing for a higher number of detectable gravitational-wave signals, and provided confirmation of all observed gravitational wave events as discussed by the authors.