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Beating the spin-down limit on gravitational wave emission from the vela pulsar

Abadie, J; Abbott, B; Hough, J; Ivanov, A; Harry, Gregory M; King, P; Kozak, D; Mailand, K; Marx, Jay; Meshkov, S; Chua, Sheon; Inta, Ra; McClelland, David; Mow-Lowry, C; Mullavey, Adam; Satterthwaite, Matthew; Scott, Susan M; Shaddock, Daniel; Slagmolen, Bram; Stefszky, Michael; Heefner, J; Hosken, Dave; Howell, E


We present direct upper limits on continuous gravitational wave emission from the Vela pulsar using data from the Virgo detector's second science run. These upper limits have been obtained using three independent methods that assume the gravitational wave emission follows the radio timing. Two of the methods produce frequentist upper limits for an assumed known orientation of the star's spin axis and value of the wave polarization angle of, respectively, 1.9 × 10-24 and 2.2 × 10-24, with 95%...[Show more]

CollectionsANU Research Publications
Date published: 2011
Type: Journal article
Source: Astrophysical Journal, The
DOI: 10.1088/0004-637X/737/2/93


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