Status of the AURIGA detector as May 2009

The detector is stationary since may 2005. Here follow a few pictures showing the AURIGA performance as gravitational wave detector.

Figure 1

Figure 1: AURIGA sensitivity, ie (single-sided) spectral noise, on 13 may 2009

Figure 2

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

Figure 3

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.