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Leo Singer

Researcher at Goddard Space Flight Center

Publications -  344
Citations -  98557

Leo Singer is an academic researcher from Goddard Space Flight Center. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 100, co-authored 326 publications receiving 76449 citations. Previous affiliations of Leo Singer include California Institute of Technology & Max Planck Society.

Papers
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Journal ArticleDOI

Search for intermediate mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo

Richard J. Abbott, +1632 more
Journal ArticleDOI

Upper Limits on Gravitational Waves from Scorpius X-1 from a Model-Based Cross-Correlation Search in Advanced LIGO Data

B. P. Abbott, +1043 more
TL;DR: In this paper, the results of a semicoherent search for continuous gravitational waves from the low-mass X-ray binary Scorpius X-1, using data from the first Advanced LIGO observing run were presented.
Journal ArticleDOI

A Fermi Gamma-ray Burst Monitor Search for Electromagnetic Signals Coincident with Gravitational-Wave Candidates in Advanced LIGO's First Observing Run

Fermi Gamma-ray Burst Monitor Team, +1156 more
TL;DR: In this article, a search for prompt gamma-ray counterparts to compact binary coalescence gravitational wave (GW) candidates from Advanced LIGO's first observing run (O1) is presented.

Localization and broadband follow-up of the gravitational-wave transient GW150914

B. P. Abbott, +1540 more
TL;DR: In this paper, the sky localization of the first observed compact binary merger is presented, where the authors describe the low-latency analysis of the LIGO data and present a sky localization map.
Journal ArticleDOI

Results of the deepest all-sky survey for continuous gravitational waves on LIGO S6 data running on the Einstein@Home volunteer distributed computing project

B. P. Abbott, +968 more
- 18 Nov 2016 - 
TL;DR: In this article, the authors report results of a deep all-sky search for periodic gravitational waves from isolated neutron stars in data from the S6 LIGO science run and set the most stringent upper limits to date on the amplitude of gravitational wave signals from the target population.