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R

R. Goetz

Researcher at University of Florida

Publications -  158
Citations -  58442

R. Goetz is an academic researcher from University of Florida. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 71, co-authored 147 publications receiving 47611 citations. Previous affiliations of R. Goetz include Florida Atlantic University & Max Planck Society.

Papers
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GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences

B. P. Abbott, +1099 more
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First Searches for Optical Counterparts to Gravitational-wave Candidate Events

M. Constancio, +924 more
TL;DR: In this paper, the authors compare the sensitivities of these observations to several model light curves from possible sources of interest, and discuss prospects for future joint GW-optical observations of this type.
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First search for nontensorial gravitational waves from known pulsars

B. P. Abbott, +1223 more
TL;DR: After searching data from the first observation run of the advanced LIGO detectors for signals at twice the rotational frequency of 200 known pulsars, no evidence of gravitational waves of any polarization is found.
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Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015-2017 LIGO Data

B. P. Abbott, +1232 more
TL;DR: In this article, the authors presented a search for gravitational waves from 222 pulsars with rotation frequencies ≳10 Hz using advanced LIGO data from its first and second observing runs spanning 2015-2017, which provides the highest-sensitivity gravitational-wave data so far obtained.
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First targeted search for gravitational-wave bursts from core-collapse supernovae in data of first-generation laser interferometer detectors

B. P. Abbott, +995 more
- 15 Nov 2016 - 
TL;DR: In this article, the authors present results from a search for gravitational-wave bursts coincident with a set of two core-collapse supernovae observed between 2007 and 2011, and present the probability of detecting signals from both astrophysically well-motivated and more speculative gravitational wave emission mechanisms as a function of distance from Earth.