Spectral line removal in the LIGO Data Anaylsis System (LDAS)

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dc.contributor.authorSearle, Antony
dc.contributor.authorScott, Susan M
dc.contributor.authorMcClelland, David
dc.date.accessioned2015-12-13T23:11:46Z
dc.date.issued2003
dc.date.updated2015-12-12T08:28:56Z
dc.description.abstractHigh power in narrow frequency bands, spectral lines, are a feature of an interferometric gravitational wave detector's output. Some lines are coherent between interferometers, in particular, the 2 km and 4 km LIGO Hanford instruments. This is of concern
dc.identifier.issn0264-9381
dc.identifier.urihttp://hdl.handle.net/1885/87741
dc.publisherInstitute of Physics Publishing
dc.sourceClassical and Quantum Gravity
dc.titleSpectral line removal in the LIGO Data Anaylsis System (LDAS)
dc.typeJournal article
local.bibliographicCitation.issue17
local.bibliographicCitation.lastpageS730
local.bibliographicCitation.startpageS721
local.contributor.affiliationSearle, Antony, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationScott, Susan M, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationMcClelland, David, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidSearle, Antony, u9719170
local.contributor.authoruidScott, Susan M, u8911327
local.contributor.authoruidMcClelland, David, u8802403
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor029904 - Synchrotrons; Accelerators; Instruments and Techniques
local.identifier.absfor010501 - Algebraic Structures in Mathematical Physics
local.identifier.ariespublicationMigratedxPub17163
local.identifier.citationvolume20
local.identifier.doi10.1088/0264-9381/20/17/315
local.identifier.scopusID2-s2.0-0142230409
local.type.statusPublished Version

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