Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/48819
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dc.contributor.author | Abbott, B. | - |
dc.contributor.author | Abbott, R. | - |
dc.contributor.author | Adhikari, R. | - |
dc.contributor.author | Ageev, A. | - |
dc.contributor.author | Allen, B. | - |
dc.contributor.author | Amin, R. | - |
dc.contributor.author | Anderson, S. | - |
dc.contributor.author | Anderson, W. | - |
dc.contributor.author | Araya, M. | - |
dc.contributor.author | Armandula, H. | - |
dc.contributor.author | Ashley, M. | - |
dc.contributor.author | Asiri, F. | - |
dc.contributor.author | Aufmuth, P. | - |
dc.contributor.author | Aulbert, C. | - |
dc.contributor.author | Babak, S. | - |
dc.contributor.author | Balasubramanian, R. | - |
dc.contributor.author | Ballmer, S. | - |
dc.contributor.author | Barish, B. | - |
dc.contributor.author | Barker, C. | - |
dc.contributor.author | Barker, D. | - |
dc.contributor.author | et al. | - |
dc.date.issued | 2005 | - |
dc.identifier.citation | Physical Review D: Particles, Fields, Gravitation and Cosmology, 2005; 72(8):082001-1-082001-22 | - |
dc.identifier.issn | 1550-7998 | - |
dc.identifier.issn | 1550-2368 | - |
dc.identifier.uri | http://hdl.handle.net/2440/48819 | - |
dc.description.abstract | We use 373 hours (≈15 days) of data from the second science run of the LIGO gravitational-wave detectors to search for signals from binary neutron star coalescences within a maximum distance of about 1.5 Mpc, a volume of space which includes the Andromeda Galaxy and other galaxies of the Local Group of galaxies. This analysis requires a signal to be found in data from detectors at the two LIGO sites, according to a set of coincidence criteria. The background (accidental coincidence rate) is determined from the data and is used to judge the significance of event candidates. No inspiral gravitational-wave events were identified in our search. Using a population model which includes the Local Group, we establish an upper limit of less than 47 inspiral events per year per Milky Way equivalent galaxy with 90% confidence for nonspinning binary neutron star systems with component masses between 1 and 3M⊙. | - |
dc.description.statementofresponsibility | B. Abbott...C. Killow...D. Ottaway...et al., LIGO Scientific Collaboration | - |
dc.language.iso | en | - |
dc.publisher | American Physical Soc | - |
dc.rights | ©2005 American Physical Society | - |
dc.source.uri | http://dx.doi.org/10.1103/physrevd.72.082001 | - |
dc.title | Search for gravitational waves from galactic and extra-galactic binary neutron stars | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1103/PhysRevD.72.082001 | - |
pubs.publication-status | Published | - |
dc.identifier.orcid | Ottaway, D. [0000-0001-6794-1591] | - |
Appears in Collections: | Aurora harvest 6 Physics publications |
Files in This Item:
File | Description | Size | Format | |
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hdl_48819.pdf | Published version | 1.61 MB | Adobe PDF | View/Open |
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