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Resolving the FIR/SMM Cosmic Background and thus Studying the High-Redshift Universe from Concordia Station

Published online by Cambridge University Press:  24 December 2009

L. Spinoglio ,
N. Epchtein ,
M. Vaccari  and
A. Franceschini
M. Vaccari*
Affiliation:
Department of Astronomy, University of Padova, Vicolo Osservatorio 3, 35122 Padova, Italy
A. Franceschini
Affiliation:
Department of Astronomy, University of Padova, Vicolo Osservatorio 3, 35122 Padova, Italy
*
mattia@mattiavaccari.net
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Abstract

The excellent observing conditions at Concordia station offer an outstanding opportunity to carry out sensitive FIR/SMM surveys of the extragalactic sky in order to resolve the Cosmic Background at these wavelengths. We outline the main standing questions about the formation and evolution of galaxies making up the FIR/SMM Cosmic Background and discuss how single-dish observations with either a 12-m or a 25-m antenna at Concordia would help in answering them.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 40: 3rd ARENA Conference: An Astronomical Observatory at CONCORDIA (Dome C, Antarctica) , 2010 , pp. 429 - 436
Copyright
© EAS, EDP Sciences, 2010

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