University of Tasmania
Browse
Siellez - Properties of the Binary Black Hole Merger GW150914.pdf (1.22 MB)

Properties of the Binary Black Hole Merger GW150914

Download (1.22 MB)
journal contribution
posted on 2023-05-21, 11:38 authored by Abbott, BP, Abbott, R, Karelle SiellezKarelle Siellez, Zweizig, J, Boyle, M, Brugmann, B, Campanelli, M, Clark, M, Hamberger, D, Kidder, LE, Kinsey, M, Laguna, P, Ossokine, S, Scheel, MA, Szilagyi, B, Teukolsky, S, Zlochower, Y
On September 14, 2015, the Laser Interferometer Gravitational-Wave Observatory (LIGO) detected a gravitational-wave transient (GW150914); we characterize the properties of the source and its parameters. The data around the time of the event were analyzed coherently across the LIGO network using a suite of accurate waveform models that describe gravitational waves from a compact binary system in general relativity.

History

Publication title

Physical Review Letters

Volume

116

Issue

24

Article number

241102

Number

241102

Pagination

1-19

ISSN

0031-9007

Department/School

School of Natural Sciences

Publisher

American Physical Soc

Place of publication

One Physics Ellipse, College Pk, USA, Md, 20740-3844

Rights statement

© 2016 The Author(s). Published by the American Physical Society under the terms of the Creative Commons Attribution 3.0 Unported (CC BY 3.0) License (https://creativecommons.org/licenses/by/3.0/). Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Repository Status

  • Open

Socio-economic Objectives

Expanding knowledge in the physical sciences

Usage metrics

    University Of Tasmania

    Exports

    RefWorks
    BibTeX
    Ref. manager
    Endnote
    DataCite
    NLM
    DC