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Maggie Tse

Researcher at Massachusetts Institute of Technology

Publications -  112
Citations -  41395

Maggie Tse is an academic researcher from Massachusetts Institute of Technology. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 53, co-authored 101 publications receiving 33596 citations. Previous affiliations of Maggie Tse include California Institute of Technology & Columbia University.

Papers
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Journal ArticleDOI

GW150914: First results from the search for binary black hole coalescence with Advanced LIGO

B. P. Abbott, +980 more
- 07 Jun 2016 - 
TL;DR: In this paper, the results of a matched-filter search using relativistic models of compact-object binaries that recovered GW150914 as the most significant event during the coincident observations between the two LIGO detectors were reported.
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The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914

B. P. Abbott, +961 more
TL;DR: In this paper, the authors report on the constraints these observations place on the rate of binary black hole coalescences, and estimate a 90% credible range of merger rates between $2$--$53 \, \mathrm{Gpc}^{-3} \mathm{yr}^{ −1}$ (comoving frame).
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
TL;DR: In this article, the authors presented the results from three gravitational-wave searches for coalescing compact binaries with component masses above 1, during the first and second observing runs of the Advanced Gravitational-wave detector network.
Journal ArticleDOI

Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914

B. P. Abbott, +1002 more
TL;DR: The transient noise backgrounds used to determine the significance of the event (designated GW150914) are described and the results of investigations into potential correlated or uncorrelated sources of transient noise in the detectors around the time of theevent are presented.
Journal ArticleDOI

Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run

B. P. Abbott, +1067 more
TL;DR: This work performs a search for the isotropic stochastic gravitational-wave background using data from Advanced Laser Interferometer Gravitational Wave Observatory's (aLIGO) first observing run, and constrain the dimensionless energy density of gravitational waves to be Ω_{0}<1.7×10^{-7} with 95% confidence.