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Corrigendum: The third post-Newtonian gravitational wave polarizations and associated spherical harmonic modes for inspiralling compact binaries in quasi-circular orbits

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dc.contributor.authorIyer, B R
dc.contributor.authorSinha, Siddhartha
dc.contributor.authorBlanchet, Luc
dc.contributor.authorGuillaume, Faye
dc.date.accessioned2013-02-01T04:54:05Z
dc.date.available2013-02-01T04:54:05Z
dc.date.issued2012-12-07
dc.descriptionRestricted Access.en
dc.identifier.citationClassical and Quantum Gravity, 2012, Vol.29, p239501en
dc.identifier.issn0264-9381
dc.identifier.issn1361-6382(Online)
dc.identifier.urihttp://hdl.handle.net/2289/5389
dc.language.isoenen
dc.publisherIOP Publishingen
dc.relation.urihttp://dx.doi.org/10.1088/0264-9381/29/23/239501en
dc.rights2012 IOP Publishingen
dc.titleCorrigendum: The third post-Newtonian gravitational wave polarizations and associated spherical harmonic modes for inspiralling compact binaries in quasi-circular orbitsen
dc.typeArticleen

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