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The data for the predicted noise power spectra for the initial and advanced LIGO detectors were taken from, Those for the VIRGO detector were supplied by Luca Gammaitoni (E-mail address: gammaitoni@perugia.infn.it);, the GEO-600 detector by Albrecht Rudiger and Kenneth Strain (E-mail address: atr@mpq.mpg.de and kstrain@physics.gla.ac.uk);, and the TAMA-300 detector by Masa-Katsu Fujimoto (E-mail address: fujimoto@gravity.mtk.nao.ac.jp)., The predicted noise power spectra for the “enhanced” LIGO detectors were supplied by Rainer Weiss (E-mail address: weiss@tristan.mit.edu).
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