LIGO Document G1000786-v1

A search for gravitational waves from a nearby neutron star

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LIGO-G1000786-v1
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G - Presentations (eg Graphics)
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Abstract:
Rapidly spinning neutron stars in our Galactic neighborhood are promising sources of quasi-monochromatic continuous gravitational waves observable by the current LIGO detectors. I describe a search done on the LIGO S5 data, looking for an isolated neutron star hypothesized to be at a distance of about 100 parsecs. This kind of search is computationally bound and is made possible by the implementation of barycentric resampling, which is described here as well.
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