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CTA site characterization: a contribution on Sky Background Brightness

Published online by Cambridge University Press:  05 March 2015

Gonzalo de la Vega
Affiliation:
ITeDA Mendoza, CNEA, CONICET, UNSAM Azopardo 313 5501 Godoy Cruz, Mendoza, Argentina email: [email protected]
Beatriz García
Affiliation:
ITeDA Mendoza, CNEA, CONICET, UNSAM Azopardo 313 5501 Godoy Cruz, Mendoza, Argentina email: [email protected]
Javier Maya
Affiliation:
ITeDA Mendoza, CNEA, CONICET, UNSAM Azopardo 313 5501 Godoy Cruz, Mendoza, Argentina email: [email protected]
Alexis Mancilla
Affiliation:
ITeDA Mendoza, CNEA, CONICET, UNSAM Azopardo 313 5501 Godoy Cruz, Mendoza, Argentina email: [email protected]
Ezequiel Rosemblat
Affiliation:
Universidad Mendoza, Mendoza, Argentina
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Abstract

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The Cherenkov Telescope Array (CTA) is an international project for which more than 1000 scientists from 27 countries work together to install two observatories, one in the southern hemisphere and the other in the north, to study gamma-ray radiation. Argentina is a candidate site for one of the observatories, and to characterize proposed sites, one must study the sky background brightness. This critical point must be studied with care. Nearest cities can be a decisive factor in determining where to locate an observatory in our times.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

Patat, F., ESO Internal Report, 2006. (http://www.eso.org/~fpatat/science/skybright/)Google Scholar
Patat, F., A&A 481 575591, 2008Google Scholar