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G. Mazzolo

Researcher at Max Planck Society

Publications -  42
Citations -  14814

G. Mazzolo is an academic researcher from Max Planck Society. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 26, co-authored 41 publications receiving 12684 citations. Previous affiliations of G. Mazzolo include Leibniz University of Hanover.

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The characterization of Virgo data and its impact on gravitational-wave searches

J. Aasi, +800 more
TL;DR: In this article, the authors present examples from the joint LIGO-GEO-Virgo GW searches to show how well noise transients and narrow spectral lines have been identified and excluded from the Virgo data.
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Searches for continuous gravitational waves from nine young supernova remnants

J. Aasi, +889 more
TL;DR: In this article, the authors describe directed searches for continuous gravitational waves in data from the sixth LIGO science data run, where the targets were nine young supernova remnants not associated with pulsars; eight of the remnants are associated with non-pulsing suspected neutron stars.
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Swift follow-up observations of candidate gravitational-wave transient events

P. A. Evans, +815 more
TL;DR: In this article, the first multi-wavelength follow-up observations of two candidate gravitational-wave (GW) transient events recorded by LIGO and Virgo in their 2009-2010 science run are presented.

Sensitivity Achieved by the LIGO and Virgo Gravitational Wave Detectors during LIGO's Sixth and Virgo's Second and Third Science Runs

J. Abadie, +797 more
TL;DR: In this article, the authors summarize the sensitivity achieved by the LIGO and Virgo detectors for low-mass compact binary coalescence (CBC) searches during the LigO's sixth science run and the Virgo's second and third science runs.
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Supplement: Localization and broadband follow-up of the gravitational-wave transient GW150914

B. P. Abbott, +1539 more
TL;DR: In this paper, the authors summarize past electromagnetic follow-up efforts as well as the organization and policy of the current EM followup program and compare the four probability sky maps produced for the gravitational-wave transient GW150914, and provide additional details of the EM follow up observations that were performed in the different bands.