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Soma Mukherjee

Researcher at University of Texas at Austin

Publications -  280
Citations -  72580

Soma Mukherjee is an academic researcher from University of Texas at Austin. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 95, co-authored 266 publications receiving 59549 citations. Previous affiliations of Soma Mukherjee include The University of Texas Rio Grande Valley & Saha Institute of Nuclear Physics.

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Journal ArticleDOI

Upper Limits on Gravitational Waves from Scorpius X-1 from a Model-Based Cross-Correlation Search in Advanced LIGO Data

B. P. Abbott, +1078 more
TL;DR: In this article, a semicoherent search for continuous gravitational waves from the low-mass X-ray binary Scorpius X-1, using data from the first Advanced LIGO observing run, was conducted over the frequency range 25-2000\,\mathrm{Hz}, spanning the current observationally constrained range of binary orbital parameters.
Journal ArticleDOI

Constraints on Cosmic Strings Using Data from the Third Advanced LIGO–Virgo Observing Run

Richard J. Abbott, +1668 more
TL;DR: In this article, the authors search for gravitational-wave signals produced by cosmic strings in the Advanced LIGO and Virgo full O3 dataset and obtain results for the first time that kink-kink collisions do not yield a detection.
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Search for gravitational wave ringdowns from perturbed black holes in LIGO S4 data

B. P. Abbott, +510 more
- 09 Sep 2009 - 
TL;DR: In this paper, the authors present a search for gravitational waves from black hole ringdown in the fourth LIGO science run S4, during which the dominant mode of perturbed black holes with masses in the range of 10M to 500M⊙, the regime of intermediate-mass black holes to distances up to 300 Mpc.
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Stacked search for gravitational waves from the 2006 SGR 1900+14 Storm

B. P. Abbott, +512 more
TL;DR: The results of a LIGO search for short-duration gravitational waves (GWs) associated with the 2006 March 29 SGR 1900+14 storm are presented in this paper.
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Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600-1000 Hz

J. Abadie, +875 more
- 04 Jun 2012 - 
TL;DR: In this paper, the authors presented the first joint search for a stochastic background using data from the LIGO and Virgo interferometers in a frequency band of 600-1000 Hz.