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Supriyo Sinha

Researcher at Stanford University

Publications -  62
Citations -  3928

Supriyo Sinha is an academic researcher from Stanford University. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 34, co-authored 62 publications receiving 3764 citations. Previous affiliations of Supriyo Sinha include Howard Hughes Medical Institute.

Papers
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An upper limit on the stochastic gravitational-wave background of cosmological origin

B. P. Abbott, +667 more
- 20 Aug 2009 - 
TL;DR: In this paper, the authors reported limits on the amplitude of the stochastic gravitational-wave background using the data from a two-year science run of the Laser Interferometer Gravitational-wave Observatory (LIGO).
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Searches for gravitational waves from known pulsars with science run 5 LIGO data

B. P. Abbott, +705 more
TL;DR: In this article, an updated search for gravitational waves from 116 known millisecond and young pulsars using data from the fifth science run of the LIGO detectors was presented, where ephemerides overlapping the run period were obtained using radio and X-ray observations.
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Search for gravitational waves from binary inspirals in S3 and S4 LIGO data

B. P. Abbott, +463 more
- 07 Mar 2008 - 
TL;DR: In this paper, a search for gravitational waves from the coalescence of compact binary systems during the third and fourth LIGO science runs was reported, which focused on gravitational waves generated during the inspiral phase of the binary evolution.
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Observation of a kilogram-scale oscillator near its quantum ground state

B. P. Abbott, +454 more
TL;DR: In this paper, the resonant frequency of a 2.7 kg pendulum mode was dynamically shifted to lie within this optimal band, where its effective temperature falls as low as 1.4 μK and its occupation number reaches about 200 quanta.
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Upper limits on gravitational wave emission from 78 radio pulsars

B. P. Abbott, +465 more
- 03 Aug 2007 - 
TL;DR: In this paper, the authors presented upper limits on the gravitational wave emission from 78 radio pulsars based on data from the third and fourth science runs of the LIGO and GEO 600 gravitational wave detectors.