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Search of S3 LIGO data for gravitational wave signals from spinning black hole and neutron star binary inspirals

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Figure

FIG. 2.Moment functions(dashed line) for the initial LIGO design noise power spectraldensity
FIG. 3 (color online).A template bank generated with minimal matchfrequencytemplates in the ¼ 0:95 using 2048 seconds of H1 data taken during S3
Figure � 3 shows a template bank generated using 2048
TABLE I.Summary of the amount of data analyzed in ourvarious data sets. In S3 we only analyze data from the LHOdetectors when both H1 and H2 are in science mode
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