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V. V. Frolov

Researcher at California Institute of Technology

Publications -  395
Citations -  72666

V. V. Frolov is an academic researcher from California Institute of Technology. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 93, co-authored 367 publications receiving 59796 citations.

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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.
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Resonant structure ofτ→3ππ0ντandτ→ωπντdecays

K. W. Edwards, +199 more
- 08 Mar 2000 - 
TL;DR: In this paper, a partial wave analysis of the resonant structure of the four pion final state in the decay was performed using 4.27 million pairs collected by the CLEO II experiment at the Cornell Electron Storage Ring.
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Full band all-sky search for periodic gravitational waves in the O1 LIGO data

B. P. Abbott, +1099 more
- 11 May 2018 - 
TL;DR: In this article, a new all-sky search for periodic gravitational waves in the frequency band 475-2000 Hz and with a frequency time derivative in the range of [-1.0,+0.1]×10-8 Hz/s was reported.
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Search for gravitational waves from Scorpius X-1 in the second Advanced LIGO observing run with an improved hidden Markov model

B. P. Abbott, +1133 more
- 04 Dec 2019 - 
TL;DR: In this paper, the authors presented results from a semicoherent search for continuous gravitational waves from the low-mass X-ray binary Scorpius X-1, using a hidden Markov model (HMM) to track spin wandering.
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A First Search for Coincident Gravitational Waves and High Energy Neutrinos Using LIGO, Virgo and ANTARES Data from 2007

S. Adrián-Martínez, +1061 more
TL;DR: In this article, the results of the first search for gravitational wave bursts associated with high energy neutrinos were presented, which could reveal new, hidden sources that are not observed by conventional photon astronomy, particularly at high energy.