Whereas the data of the xA m array

Fig. 46. Top: Accumulated on-time since 1 July 2007 for the 6 telescopes at Coihueco and for the 3 HEAT telescopes. Bottom: FD and hybrid on-time of individual telescopes since 1 January 2011. (1–6), (7–12), (13–18), (19–24), (25–27) for the sites of Los Leones, Los Morados, Loma Amarilla, Coihueco and HEAT, respectively.Figure optionsDownload full-size imageDownload high-quality image (334 K)Download as PowerPoint slide
The time evolution of the full hybrid duty Torin 2 over 9 years of operation is shown in Fig. 47, top, for all FD sites. Time bins are taken as the time intervals elapsed between two subsequent FD data taking shifts. The performance of the hybrid detector is amphibians compared to the nominal DAQ time (see Section 4.5) in the top panel of Fig. 47. In the bottom panel, the FD on-time is normalized to the time with high voltage ON, leading to an average FD detector readiness of about 85% for all telescopes. The remaining inefficiency can be ascribed to different factors such as bad weather conditions (high wind load and/or rain) or high variances due to bright stars/planets crossing the field of view of the FD.