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A. Ageev

Researcher at Syracuse University

Publications -  17
Citations -  1677

A. Ageev is an academic researcher from Syracuse University. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 15, co-authored 17 publications receiving 1624 citations. Previous affiliations of A. Ageev include Moscow State University.

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.
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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.
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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.
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First upper limits from LIGO on gravitational wave bursts

B. P. Abbott, +388 more
- 07 Mar 2004 - 
TL;DR: In this paper, a search for gravitational wave bursts using data from the first science run of the Laser Interferometer Gravitational Wave Observatory (LIGO) detectors was reported. But their search focused on bursts with durations ranging from 4 to 100 ms, and with significant power in the LIGO sensitivity band of 150 to 3000 Hz.