Difference: Galery (2 vs. 3)
Revision 32011-03-05 - GergelyDebreczeni
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| SNR distribution of a 1.5 - 3.0 MSun component mass non-spinning, circular binary inspiral waveforms injected at 5 Mpc distance and reconstructed with a template bank of the same kind using simulated PSD at nominal detector | ||||||||||
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The noise curve of the Virgo detector in the 40 - 2048 Hz region with fitted model curve. | |||||||||
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