Characterization of atmospheric properties at the future sites of the Cherenkov Telescope Array
Jan Ebr, Du\v{s}an Mand\'at, Miroslav Pech, Ladislav Chytka, Jakub, Jury\v{s}ek, Michael Prouza, Petr Jane\v{c}ek, Petr Tr\'avn\'i\v{c}ek,, Ji\v{r}\'i Bla\v{z}ek, Tomasz Bulik, Marek Cieslar, Mariusz Suchenek,, Vincenzo Rizi, Ermanno Pietropaolo, Marco Iarlori, Carla Aramo

TL;DR
This paper provides a comprehensive characterization of atmospheric conditions at the future Cherenkov Telescope Array sites, using various instruments and data sources to inform optimal telescope operation.
Contribution
It offers a detailed atmospheric profile of the sites, combining multiple measurement techniques and ongoing data collection efforts to support future telescope deployment.
Findings
Cloudiness monitored over several years at both sites.
Aerosol optical depth measured since 2016 at the southern site.
Vertical aerosol and water vapor profiles obtained with Raman lidar.
Abstract
Advanced knowledge of the detailed atmospheric properties of both the future sites of the Cherenkov Telescope Array is essential in preparation of the arrival of the first scientific data. Meteorological variables are studied using a dedicated characterization station installed at the southern site in Chile and a wealth of data from existing observatories around the northern site on the La Palma island. Campaigns using radiosondes launched on balloons are foreseen to complement these data in the near future. Cloudiness during the night has been continuously monitored at both sites for several years using All-sky Cameras which assess the presence of clouds based on detection of stars. The integrated aerosol optical depth over the southern site has been measured using a Sun/Moon Photometer since 2016 and the small robotic FRAM telescope since 2017; identical instruments have been deployed…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Atmospheric Ozone and Climate
