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During the flight, the gondola pendulates and does not rotate at
constant speed, we therefore have to reconstruct off line the direction
pointed by each bolometer for each sample. This is done using a
stellar sensor telescope that is attached to the gondola and points in
the same direction as the bolometers. The stellar sensor focal plane
contains 48 photodiodes whose signal exhibits a peak whenever they
cross a star. We therefore obtained an observed star catalog that is
compared with a real one in order to give the pointing solution. Our
pointing accuracy is estimated to be around one arcminute.
Jean-Christophe Hamilton ISN
2001-12-01