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First targeted search for gravitational-wave bursts from core-collapse supernovae in data of first-generation laser interferometer detectors

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Figure

TABLE I.Core-collapse supernovae selected as triggers for the gravitational-wave search described in this paper
TABLE II.Overview of GW interferometer science runs from which we draw data for our search
FIG. 2.Noise amplitude spectral densities of the GW interfer-ometers whose data are analyzed for SNe 2007gr and 2011dh (seeSec
FIG. 3.False Alarm Probability [FAP, Equationbackground noise. The left panel shows the FAP distribution determined by thedetector network (cf
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