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C. Hardham

Researcher at Stanford University

Publications -  29
Citations -  2361

C. Hardham is an academic researcher from Stanford University. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 22, co-authored 29 publications receiving 2209 citations.

Papers
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Journal ArticleDOI

Detector description and performance for the first coincidence observations between LIGO and GEO

B. P. Abbott, +423 more
TL;DR: For 17 days in August and September 2002, the LIGO and GEO interferometer gravitational wave detectors were operated in coincidence to produce their first data for scientific analysis.
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Setting upper limits on the strength of periodic gravitational waves from PSR J1939+2134 using the first science data from the GEO 600 and LIGO detectors

B. P. Abbott, +376 more
- 15 Apr 2004 - 
TL;DR: In this article, a model emission mechanism is used to interpret the limits as a constraint on the pulsar's equatorial ellipticity, and two independent analysis methods are used and are demonstrated in two independent methods: a frequency domain method and a time domain method.
Journal ArticleDOI

Analysis of LIGO data for gravitational waves from binary neutron stars

B. P. Abbott, +223 more
- 15 Jun 2004 - 
TL;DR: In this paper, the authors report on a search for gravitational waves from coalescing compact binary systems in the Milky Way and the Magellanic Clouds using data taken by two of the three LIGO interferometers.
Journal ArticleDOI

Limits on gravitational-wave emission from selected pulsars using LIGO data.

B. P. Abbott, +407 more
TL;DR: The unprecedented sensitivity of the detectors allows us to set strain upper limits as low as a few times 10(-24), which translate into limits on the equatorial ellipticities of the pulsars, which are smaller than 10(-5) for the four closest pulsars.
Journal ArticleDOI

Searching for a stochastic background of gravitational waves with the laser interferometer gravitational-wave observatory

B. Abbott, +411 more
TL;DR: In this article, the amplitude of a stochastic background of gravitational waves has been shown to be ΩGW × [H0/(72 km s−1 Mpc−1)]2 < 6.5 × 10-5.