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An Instrument Devoted to the Study of mm/sub-mm Galactic Emission at Dome C
Published online by Cambridge University Press: 25 April 2016
Abstract
An experiment has been developed in order to map the submillimetre Galactic emission at four different wavelengths between 400 μm and 2 mm at an angular scale of 1°. A binocular telescope system has been realised by means of two off-axis wobbling parabolic mirrors, each one coupled to a two-channel 3He photometer. A first run of observations from Dome C is planned for the Antarctic summer 1995–96.
Keywords
- Type
- The First JACARA International Antarctic Astronomy Meeting
- Information
- Publications of the Astronomical Society of Australia , Volume 13 , Issue 1 , January 1996 , pp. 44 - 47
- Copyright
- Copyright © Astronomical Society of Australia 1996
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