Speaker
Description
The Cherenkov Telescope Array (CTA) will have unprecedented accuracy and sensitivity, affording us the ability to understand the mysteries of the high energy universe. This unprecedented accuracy does however also force us to adapt current calibration procedures, or indeed pioneer new techniques, to ensure the envisaged CTA performance. CTA will infer the energy of the gamma-rays it detects by the amount of Cherenkov radiation it observes. As such, the optical efficiency of the telescopes needs to be monitored and also its wavelength dependent degradation, which might be different for different telescope types, needs to be determined. Based on the results of a feasibility study, a novel cross-calibration method with an unmanned aerial vehicle (UAV) was tested on the H.E.S.S. telescope array, leading to the World's first cross-calibration of an Imaging Atmospheric Cherenkov Telescope (IACT) array with a single light source. In this talk, we present the cross-calibration results from a first campaign in which we determine the relative optical efficiencies of the four HESS-I telescopes by successfully recording light from the UAV-mounted nanosecond pulsed UV light source simultaneously in all four telescopes. In addition, we show that the UAV data can be used to monitor the pointing accuracy at least at the level of tens of arcseconds and we give an outlook on other potential use cases of the UAV such as the monitoring of the atmospheric state.
Keywords
Gamma-ray; IACT; calibration; cross-calibration; optical efficiency; UAV;
| Subcategory | Experimental Methods & Instrumentation |
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