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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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Implications for the origin of GRB 051103 from LIGO observations

J. Abadie, +574 more
TL;DR: In this paper, the results of a LIGO search for gravitational waves (GWs) associated with GRB 051103, a short-duration hard-spectrum gamma-ray burst (GRB) whose electromagnetically determined sky position is coincident with the spiral galaxy M81, which is 3.6 Mpc from Earth.
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Search for gravitational waves associated with gamma-ray bursts during LIGO science run 6 and Virgo science runs 2 and 3

J. Abadie, +807 more
TL;DR: The results of a search for gravitational waves associated with 154 gamma-ray bursts (GRBs) that were detected by satellite-based gamma ray experiments in 2009-2010, during the sixth LIGO science run and the second and third Virgo science runs are presented in this article.
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Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817

B. P. Abbott, +1138 more
TL;DR: In this paper, the authors revisited the binary neutron star coalescence with a focus on longer signal durations up until the end of the Second Advanced LIGO-Virgo Observing run, 8.5 days after the coalescence of GW170817.
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An improved analysis of GW150914 using a fully spin-precessing waveform model

B. P. Abbott, +970 more
TL;DR: In this paper, a 15-dimensional precessing-spin waveform model (precessing EOBNR) was developed within the EOB formalism for GW150914.
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First low-latency LIGO+Virgo search for binary inspirals and their electromagnetic counterparts

J. Abadie, +876 more
TL;DR: In this article, the first low-latency search for gravitational-waves from binary inspirals in LIGO and Virgo data was conducted, and the resulting triggers were sent to electromagnetic observatories for followup.