A thermal IR large scale survey from Antarctica

Details A thermal IR large scale survey from Antarctica A thermal IR large scale survey from Antarctica

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..451e&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

Physics

Infrared, Survey

Scientific paper

We describe a project to achieve a large scale, high angular resolution, ultra deep survey in the 2.3-10 μm range from the Italo-French Antarctic Station CONCORDIA at Dôme C. It would extend the recently achieved 2-μm surveys toward a still little explored spectral range at large scale. A passively cooled 3-meter collector equipped with a mosaic of arrays would provide better sensitivity and angular resolution than IRAC on board Spitzer and the WISE mission, and single out new targets for Herschel, ALMA and the JWST. The new proposed instrument will be extremely powerful, e.g., for the quest of very low luminosity stars, extreme AGB-stars, deep exploration of highly obscured regions in galaxies.

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