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Searching for gravitational waves from known pulsars

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  • LIGO Scientific Collaboration
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<mark>Journal publication date</mark>1/09/2005
<mark>Journal</mark>Classical and Quantum Gravity
Issue number18
Volume22
Number of pages6
Pages (from-to)S1277-S1282
Publication StatusPublished
<mark>Original language</mark>English

Abstract

We present upper limits on the amplitude of gravitational waves from 28 isolated pulsars using data from the second science run of LIGO. The results are also expressed as a constraint on the pulsars' equatorial ellipticities. We discuss a new way of presenting such ellipticity upper limits that takes account of the uncertainties of the pulsar moment of inertia. We also extend our previous method to search for known pulsars in binary systems, of which there are about 80 in the sensitive frequency range of LIGO and GEO 600.