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

Autor: Tovmassian, G., Hernandez, M.-S., Ochoa, J. L., Ernenwein, J.-P., Mandat, D., Pech, M., Frayn, I.P., Colorado, E., Murillo, Jose Manuel, Ceseña, U., Garcia, B., H. Lee, W., Bulik, T., Garczarczyk, M., Fruck, C., Costantini, H., Cieslar, M., Aune, T., Vincent, S., Carr, J., Serre, N., Janecek, P., Haefner, D., Cesena, U., Lee, W. H.

Publikováno v: Publications of the Astronomical Society of the Pacific
Publications of the Astronomical Society of the Pacific, 2016, 128 (961), pp.035004. ⟨10.1088/1538-3873/128/961/035004⟩
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⟩
Publications of the Astronomical Society of the Pacific 128(961), 035004 (2016). doi:10.1088/1538-3873/128/961/035004

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 fr

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