S-Cam is a cryogenic camera developed within the Astrophysics Division of E
SA Space Science Department. The camera has been designed as a technology d
emonstrator, aiming to prove the potential of a new generation of single-ph
oton counting detectors based on Superconducting Tunnel Junctions (STJs), T
his article provides an overview of the cryogenic detector development, a d
escription of the S-Cam system and a summary of the results obtained both d
uring testing at ESTEC and during actual observations at the William Hersch
el Telescope in La Palma (Canary Islands, Spain). Initial observations were
performed on the Crab pulsar, a neutron star about 10 km in diameter and a
bout 6000 light years from Earth, with a weight equal to that of our Sun an
d spinning with a period of 33 msec.