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Dharamveer Singh

Researcher at Indian Institute of Technology Bombay

Publications -  193
Citations -  6844

Dharamveer Singh is an academic researcher from Indian Institute of Technology Bombay. The author has contributed to research in topics: Asphalt & LIGO. The author has an hindex of 26, co-authored 170 publications receiving 4407 citations. Previous affiliations of Dharamveer Singh include University of Oklahoma & Indian Institutes of Technology.

Papers
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GW190814: Gravitational Waves from the Coalescence of a 23 M$_\odot$ Black Hole with a 2.6 M$_\odot$ Compact Object

R. Abbott, +1254 more
TL;DR: In this article, the authors reported the observation of a compact binary coalescence involving a 22.2 -24.3 magnitude black hole and a compact object with a mass of 2.50 -2.67 magnitude.
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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, +1350 more
- 09 Jun 2021 - 
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.
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.
Journal ArticleDOI

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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Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521.

R. Abbott, +1254 more
TL;DR: The GW190521 signal as mentioned in this paper is consistent with a binary black hole merger source at redshift 0.8 with unusually high component masses, and shows mild evidence for spin-induced orbital precession.