A Bayesian search for gravitational waves from the Vela pulsar in Virgo VSR2 data

C. Gill*, Sheon Chua, Andrew Wade, David McClelland, Susan Scott, Ping Lam, Daniel Shaddock

*Corresponding author for this work

    Research output: Contribution to journalConference articlepeer-review

    1 Citation (Scopus)

    Abstract

    The Virgo detector undertook its second science run (VSR2) from July 2009 to January 2010, providing unprecedented sensitivity to gravitational waves at frequencies below 40 Hz. The VSR2 dataset presented an ideal opportunity [1] to search for gravitational waves from the Vela pulsar (B0833-45, J0835-4510), for which gravitational wave emission is expected at ∼ 22 Hz assuming it is a non axi-symmetric rotator. We give a summary of the results obtained in [1], describing the Bayesian method more fully and presenting further details of the data used.

    Original languageEnglish
    Article number012039
    JournalJournal of Physics: Conference Series
    Volume363
    Issue number1
    DOIs
    Publication statusPublished - 2012
    Event9th Edoardo Amaldi Conference on Gravitational Waves, Amaldi 9 and the 2011 Numerical Relativity - Data Analysis Meeting, NRDA 2011 - Cardiff, United Kingdom
    Duration: 10 Jul 201115 Jul 2011

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