The Pierre Auger Observatory surface detector array

Details The Pierre Auger Observatory surface detector array The Pierre Auger Observatory surface detector array

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spie.4858..131b&link_type=abstract

Particle Astrophysics Instrumentation. Edited by Peter W. Gorham. Proceedings of the SPIE, Volume 4858, pp. 131-136 (2003).

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Auger Observatory southern site's surface detector will consist of
1600 water Cerenkov detectors spaced 1.5 km apart on a 3000
km2 site in Mendoza, Argentina. A discussion of the design
and results from deployment of an engineering array are presented.

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