G. Dalloglio et al., AN INSTRUMENT DEVOTED TO THE STUDY OF MM SUB-MM GALACTIC EMISSION AT DOME-C/, Publications of the Astronomical Society of Australia, 13(1), 1996, pp. 44-47
An experiment has been developed in order to map the submillimetre Gal
actic emission at four different wavelengths between 400 mu m and 2 mm
at an angular scale of 1 degrees. A binocular telescope system has be
en realised by means of two off-axis wobbling parabolic mirrors, each
one coupled to a two-channel He-3 photometer. A first run of observati
ons from Dome C is planned for the Antarctic summer 1995-96.