SUBMM/FIR ASTRONOMY IN ANTARCTICA POTENTIAL FOR A LARGE TELESCOPE FACILITY

Abstract. Preliminary site testing datasets suggest that Dome C in Antarctica is one of the best sites on Earth for astronomical observations in the 200 to 500-µm regime, i.e. for far-infrared (FIR) and submillimetre (submm) astronomy. We present an overview of potential science cases that could be...

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Bibliographic Details
Main Authors: H. Zinnecker, H. Rauer, N. Epchtein (eds, V. Minier, L. Olmi, P. -o. Lagage, L. Spinoglio, G. A. Dur, D. Galilei, H. Gallée, C. Kramer, D. Marrone, E. Pantin, N. Schneider, N. Tothill, L. Valenziano, C. Veyssière
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published:
Subjects:
Antarc*
Antarctica
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.313.505
http://arxiv.org/pdf/0805.2487v1.pdf
Description
Summary:Abstract. Preliminary site testing datasets suggest that Dome C in Antarctica is one of the best sites on Earth for astronomical observations in the 200 to 500-µm regime, i.e. for far-infrared (FIR) and submillimetre (submm) astronomy. We present an overview of potential science cases that could be addressed with a large telescope facility at Dome C. This paper also includes a presentation of the current knowledge about the site characterics in terms of atmospheric transmission, stability, sky noise and polar constraints on telescopes. Current and future site testing campaigns are finally described. The participants of the ARENA workshop on Submillimetre Far-InfraRed Astronomy from

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