S-Cam is a cryogenic camera for ground-based astronomy using superconductin
g tunnel junctions (STJ's). It has been designed as a technology demonstrat
or, aiming to prove the potential of a new generation of single photon-coun
ting detectors at a ground-based telescope. The camera is based on a 6 x 6
array of Ta-Al Josephson junctions, operating at about 350 mK and individua
lly read nut. Fur each detected photon, the absorption position, the arriva
l time, and the corresponding energy are measured, In this paper, we provid
e an overview of the cryogenic detector performance, a description of the S
-Cam system, and a summary of the results obtained both during testing at E
STEC and during actual observations at the William Herschel Telescope (WHT)
in La Palma, Spain. Initial astronomical observations were performed on th
e Crab pulsar, a neutron star spinning with a period of 33 msec at about 60
00 light years from Earth.