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Jesper Munch

Researcher at University of Adelaide

Publications -  385
Citations -  80177

Jesper Munch is an academic researcher from University of Adelaide. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 99, co-authored 374 publications receiving 65349 citations. Previous affiliations of Jesper Munch include Institut des Hautes Études Scientifiques & Max Planck Society.

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Journal ArticleDOI

Erratum: Search for gravitational waves from binary black hole inspiral, merger, and ringdown (Physical Review D - Particles, Fields, Gravitation and Cosmology (2011) 83 (122005))

J. Abadie, +723 more
- 20 Sep 2012 - 
TL;DR: Abadie et al. as mentioned in this paper search for gravitational waves from binary black hole inspiral, merger, and ringdown, Phys. Rev. D 83, 122005 (2011).
Posted Content

Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run

Richard J. Abbott, +1376 more
TL;DR: In this paper, the authors search for signatures of gravitational lensing in the gravitational-wave signals from compact binary coalescences detected by Advanced LIGO and Advanced Virgo during O3a, the first half of their third observing run.
Journal ArticleDOI

Observation of optical torsional stiffness in a high optical power cavity

TL;DR: In this paper, the authors proposed a method for using the Australian Research Council and the United States National Science Foundation NSF Grant Nos. No. 0PHY-0555453 and No. 757968.
Journal ArticleDOI

Feedback control of thermal lensing in a high optical power cavity.

TL;DR: The results show that feedback control is feasible to compensate the strong thermal lensing expected to occur in advanced laser interferometric gravitational wave detectors and could cause difficulties with the control of parametric instabilities.
Journal ArticleDOI

Holographic correction of large telescope primaries by proximal, off-axis beacons

TL;DR: Compact telescope configurations incorporating a holographic correction of large, low-quality primary collectors are demonstrated and the reduction of additional off-axis aberrations introduced by the method is also demonstrated.