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Kipp Cannon

Researcher at University of Tokyo

Publications -  270
Citations -  72438

Kipp Cannon is an academic researcher from University of Tokyo. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 91, co-authored 254 publications receiving 58717 citations. Previous affiliations of Kipp Cannon include University of Toronto & University of Wisconsin–Milwaukee.

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Journal ArticleDOI

First search for gravitational waves from known pulsars with advanced LIGO

B. P. Abbott, +1039 more
TL;DR: In this paper, the results of searches for gravitational waves from 200 pulsars using data from the first observing run of the Advanced LIGO detectors were presented, and they were able to set the most constraining upper limits yet on their gravitational-wave amplitudes and ellipticities.
Journal ArticleDOI

Constraints on cosmic strings using data from the first Advanced LIGO observing run

B. P. Abbott, +1042 more
- 08 May 2018 - 
TL;DR: In this article, an analysis conducted to specifically search for gravitational-wave bursts from cosmic string loops in the data of Advanced LIGO 2015-2016 observing run (O1) was conducted.
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All-sky search for gravitational-wave bursts in the first joint LIGO-GEO-Virgo run

J. Abadie, +667 more
- 05 May 2010 - 
TL;DR: In this paper, the authors presented results from an all-sky search for unmodeled gravitational-wave bursts in the data collected by the LIGO, GEO 600 and Virgo detectors between November 2006 and October 2007.
Journal ArticleDOI

All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

B. P. Abbott, +1225 more
- 08 Jul 2019 - 
TL;DR: In this article, the results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast spinning neutron stars with an asymmetry around their rotation axis, were presented.
Journal ArticleDOI

Evryscope science: exploring the potential of all-sky gigapixel-scale telescopes

TL;DR: The Evryscope as discussed by the authors is an under-construction 780 MPix telescope which is capable of detecting transiting exoplanets around every solar-type star brighter than mV = 12, providing at least few-millimagnitude photometric precision in longterm light curves.