Infrared monitoring of the sky background emission above Dome C

Details Infrared monitoring of the sky background emission above Dome C Infrared monitoring of the sky background emission above Dome C

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sf2a.conf..153e&link_type=abstract

SF2A-2004: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 14-18, 2004. Edited by F. Combes, D. Barret

Astronomy and Astrophysics

Astrophysics

Scientific paper

The near-IR sky emission properties above Dome C are still poorly known. They are currently estimated using numerical models or extrapolations of the South Pole data. We present a simple device that would start a monitoring of the sky background in the K-short and K-dark bands, in Summer 2004-5. These data will be essential for the definition of the specifications of future wide field telescopes and interferometers at CONCORDIA.

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