Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

Limits on Gravitational-Wave Emission from Selected Pulsars Using LIGO Data

Simple item page
dc.contributor.authorCusack, B J
dc.contributor.authorMcClelland, David
dc.contributor.authorScott, Susan M
dc.contributor.authorSearle, Antony
dc.contributor.authorHeefner, J
dc.contributor.authorHeurs, M
dc.contributor.authorHough, J
dc.contributor.authorIvanov, A
dc.date.accessioned2015-12-13T22:48:24Z
dc.date.available2015-12-13T22:48:24Z
dc.date.issued2005
dc.date.updated2016-06-14T08:37:31Z
dc.description.abstractWe place direct upper limits on the amplitude of gravitational waves from 28 isolated radio pulsars by a coherent multidetector analysis of the data collected during the second science run of the LIGO interferometric detectors. These are the first direct
dc.identifier.issn0031-9007
dc.identifier.urihttp://hdl.handle.net/1885/80088
dc.publisherAmerican Physical Society
dc.sourcePhysical Review Letters
dc.subjectKeywords: Coherent multidetector analysis; Gravitational waves; Gravitational-wave emission; Gravitational-wave signals; Interferometric detectors; Radio observation; Radio pulsars; Strain limit; Upper limits; Gravitation; Gravity waves
dc.titleLimits on Gravitational-Wave Emission from Selected Pulsars Using LIGO Data
dc.typeJournal article
local.bibliographicCitation.issue18
local.bibliographicCitation.lastpage6
local.bibliographicCitation.startpage181103/1
local.contributor.affiliationCusack, B J, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationMcClelland, David, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationScott, Susan M, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSearle, Antony, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationHeefner, J, California Institute of Technology
local.contributor.affiliationHeurs, M, University of Hannover
local.contributor.affiliationHough, J, University of Glasgow
local.contributor.affiliationIvanov, A, California Institute of Technology
local.contributor.authoruidCusack, B J, u4022214
local.contributor.authoruidMcClelland, David, u8802403
local.contributor.authoruidScott, Susan M, u8911327
local.contributor.authoruidSearle, Antony, u9719170
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.absfor029904 - Synchrotrons; Accelerators; Instruments and Techniques
local.identifier.ariespublicationMigratedxPub8418
local.identifier.citationvolume94
local.identifier.doi10.1103/PhysRevLett.94.181103
local.identifier.scopusID2-s2.0-76249123224
local.type.statusPublished Version

Downloads

Collections

ANU Research Publications

DSpace software copyright © 2002-2026 LYRASIS