Astroclimatic Characterization of Vallecitos: A candidate site for the Cherenkov Telescope Array at San Pedro Martir

Abstract : We conducted an 18 month long study of the weather conditions of the Vallecitos, a proposed site in Mexico to harbor the northern array of the Cherenkov Telescope Array (CTA). It is located in Sierra de San Pedro Martir (SPM) a few kilometers away from Observatorio Astron\'omico Nacional. The study is based on data collected by the ATMOSCOPE, a multi-sensor instrument measuring the weather and sky conditions, which was commissioned and built by the CTA Consortium. Additionally, we compare the weather conditions of the optical observatory at SPM to the Vallecitos regarding temperature, humidity, and wind distributions. It appears that the excellent conditions at the optical observatory benefit from the presence of microclimate established in the Vallecitos.
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Publications of the Astronomical Society of the Pacific, Astronomical Society of the Pacific, 2016, 128 (961), pp.035004. 〈10.1088/1538-3873/128/961/035004〉
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Soumis le : lundi 9 janvier 2017 - 13:48:19
Dernière modification le : jeudi 18 janvier 2018 - 01:56:56

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G. Tovmassian, M.-S. Hernandez, J. L. Ochoa, J.-P. Ernenwein, D. Mandat, et al.. Astroclimatic Characterization of Vallecitos: A candidate site for the Cherenkov Telescope Array at San Pedro Martir. Publications of the Astronomical Society of the Pacific, Astronomical Society of the Pacific, 2016, 128 (961), pp.035004. 〈10.1088/1538-3873/128/961/035004〉. 〈in2p3-01429978〉

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