Sensitivities of alternate LISA configurations

Details Sensitivities of alternate LISA configurations Sensitivities of alternate LISA configurations

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cqgra..18.4059a&link_type=abstract

Classical and Quantum Gravity, Volume 18, Issue 19, pp. 4059-4065 (2001).

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10

Scientific paper

LISA can be considered as six proof masses, pairwise Doppler tracked with one-way optical links. An appropriate combination of these one-way Doppler links can cancel the principal noise sources (laser phase noise and optical bench motion noise). Here we compute the gravitational wave sensitivities for the baseline Michelson combination and for several other LISA data combinations which also cancel the leading noise.

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