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Angular resolution of the LISA gravitational wave detector

PHYSICAL REVIEW D, no. 12 (1998): 7089-7102

Cited by: 66|Views1

Abstract

We calculate the angular resolution of the planned LISA detector, a space-based laser interferometer for measuring low-frequency gravitational waves from galactic and extragalactic sources. LISA is not a pointed instrument; it is an all-sky monitor with a quadrupolar beam pattern. LISA will measure simultaneously both polarization compone...More

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