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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

G. Dall’Oglio ,
A. Miriametro ,
G. Morgante ,
L. Pizzo  and
L. Valenziano
G. Dall’Oglio
Affiliation:
Università di Roma III, Dipartimento di Fisica, P.le Aldo Moro 2, I-00185 Roma, Italy. dalloglio@vaxrom.roma1.infn.it
A. Miriametro
Affiliation:
Università di Roma ‘La Sapienza’, Dipartimento di Fisica, P.le Aldo Moro 2, I-00185 Roma, Italy
G. Morgante
Affiliation:
Università di Roma ‘La Sapienza’, Dipartimento di Fisica, P.le Aldo Moro 2, I-00185 Roma, Italy
L. Pizzo
Affiliation:
CNR-TESRE, Via P. Gobetti 101, I-40129 Bologna, Italy
L. Valenziano
Affiliation:
Università di Perugia, Dipartimento di Fisica, Via A. Pascoli, I-06126 Perugia, Italy
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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

Galactic emissionAntarctic Plateau
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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References

Andreani, P., et al. 1991, ApJ, 375, 148 CrossRefGoogle Scholar
Dall’Oglio, G., et al. 1992, Exp. Astron., 2, 275 CrossRefGoogle Scholar
Wright, E. L., et al. 1991, ApJ, 381, 200 CrossRefGoogle Scholar