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  Improved Hough search for gravitational wave pulsars

Krishnan, B., & Sintes, A. M. (2006). Improved Hough search for gravitational wave pulsars. Journal of Physics: Conference Series, 32, 206-211.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4BC7-4 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4BC9-F
Genre: Conference Paper

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0601081.pdf (Preprint), 122KB
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 Creators:
Krishnan, Badri1, Author              
Sintes, Alicia M.1, Author              
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              

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 Abstract: We describe an improved version of the Hough transform search for continuous gravitational waves from isolated neutron stars assuming the input to be short segments of Fourier transformed data. The method presented here takes into account possible non-stationarities of the detector noise and the amplitude modulation due to the motion of the detector. These two effects are taken into account for the first stage only, i.e. the peak selection, to create the time-frequency map of our data, while the Hough transform itself is performed in the standard way.

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 Dates: 2006
 Publication Status: Published in print
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Title: Sixth Edoardo Amaldi Conference on Gravitational Waves
Place of Event: Bankoku Shinryoukan, Okinawa, Japan
Start-/End Date: 2005-06-20 - 2005-06-24

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Title: Journal of Physics: Conference Series
Source Genre: Journal
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Pages: - Volume / Issue: 32 Sequence Number: - Start / End Page: 206 - 211 Identifier: -