scispace - formally typeset
D

David H. Shoemaker

Researcher at Massachusetts Institute of Technology

Publications -  262
Citations -  39596

David H. Shoemaker is an academic researcher from Massachusetts Institute of Technology. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 87, co-authored 261 publications receiving 32246 citations. Previous affiliations of David H. Shoemaker include Centre national de la recherche scientifique & Laser Interferometer Gravitational Wave Observatory.

Papers
More filters
Journal ArticleDOI

GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

B. P. Abbott, +1065 more
TL;DR: The magnitude of modifications to the gravitational-wave dispersion relation is constrain, the graviton mass is bound to m_{g}≤7.7×10^{-23} eV/c^{2} and null tests of general relativity are performed, finding that GW170104 is consistent with general relativity.
Journal ArticleDOI

GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

B. P. Abbott, +1148 more
- 04 Sep 2019 - 
TL;DR: In this paper, the authors presented the results from three gravitational-wave searches for coalescing compact binaries with component masses above 1 Ma during the first and second observing runs of the advanced GW detector network.
Journal ArticleDOI

LIGO: The Laser Interferometer Gravitational-Wave Observatory.

TL;DR: The goal of the Laser Interferometer Gravitational-Wave Observatory (LIGO) Project is to detect and study astrophysical gravitational waves and use data from them for research in physics and astronomy.
Journal ArticleDOI

Characterization of the LIGO detectors during their sixth science run

J. Aasi, +887 more
TL;DR: In this paper, the authors review the performance of the LIGO instruments during this epoch, the work done to characterize the detectors and their data, and the effect that transient and continuous noise artefacts have on the sensitivity of the detectors to a variety of astrophysical sources.