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Status of the AURIGA detector as May 2009 |
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The detector is stationary since may 2005. Here follow a few pictures showing the AURIGA performance as gravitational wave detector. |
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Figure 1 |
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| Figure 1: AURIGA sensitivity, ie (single-sided) spectral noise, on 13 may 2009 | |
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Figure 2 |
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Figure2: cumulative distribution of delta-like events from Nov 15th 2005 to Jan 3rd 2007: in ordinates the total number of events with SNR larger than the SNR in abscissa |
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Figure 3 |
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| Figure 3: AURIGA antenna pattern in ECEF coordinates for incoming gravitational wave with optimal orientation | |
For a history of the AURIGA status follow this link.