Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/59649
Citations
Scopus Web of Science® Altmetric
?
?
Type: Journal article
Title: Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO's fifth science run
Author: Brooks, A.
Hosken, D.
Munch, J.
Ottaway, D.
Veitch, P.
Abbott, B.
Abbott, R.
Adhikari, R.
Ajith, P.
Allen, B.
Allen, G.
Amin, R.
Anderson, S.
Anderson, W.
Arain, M.
Araya, M.
Armandula, H.
Armor, P.
Aso, Y.
Aston, S.
et al.
Citation: Physical Review. D. Particles, Fields, Gravitation and Cosmology, 2009; 80(4):7101-1-7101-5
Publisher: American Physical Soc
Issue Date: 2009
ISSN: 1550-7998
1550-2368
Statement of
Responsibility: 
B. Abbott... D. J. Hosken... J. Munch... D. J. Ottaway... P. J. Veitch...et al. (LIGO Scientific Collaboration)
Abstract: We report on a search for gravitational waves from coalescing compact binaries, of total mass between 2 and 35M⊙, using LIGO observations between November 14, 2006 and May 18, 2007. No gravitational-wave signals were detected. We report upper limits on the rate of compact binary coalescence as a function of total mass. The LIGO cumulative 90%-confidence rate upper limits of the binary coalescence of neutron stars, black holes and black hole-neutron star systems are 1.4×10-2, 7.3×10-4 and 3.6×10-3  yr-1 L10-1, respectively, where L10 is 1010 times the blue solar luminosity.
Rights: ©2009 American Physical Society
RMID: 0020092444
DOI: 10.1103/PhysRevD.80.047101
Appears in Collections:Physics publications
Environment Institute publications

Files in This Item:
File Description SizeFormat 
hdl_59649.pdfPublished version401.71 kBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.