An instrument devoted to the study of mm/sub-mm Galactic emission at Dome C

Astronomy and Astrophysics – Astronomy

Scientific paper

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Galactic Emission

Scientific paper

An experiment has been developed in order to map the sub-millimetre Galactic emission at four different wavelengths between 400 microns and 2 mm at an angular scale of 1 deg. A binocular telescope system has been realised by means of two off-axis wobbling parabolic mirrors, each one coupled to a two-channel helium-3 photometer. A first run of observations from Dome C is planned for the Antarctic summer 1995-96.

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