Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array

Details Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array

2007-02-19

arxiv.org/abs/astro-ph/0702480v1

Astronomy and Astrophysics

Astrophysics

6 pages

Scientific paper

10.1051/eas:2007114

Submillimetre/TeraHertz (e.g. 200, 350, 450 microns) astronomy is the prime technique to unveil the birth and early evolution of a broad range of astrophysical objects. A major obstacle to carry out submm observations from ground is the atmosphere. Preliminary site testing and atmospheric transmission models tend to demonstrate that Dome C could offer the best conditions on Earth for submm/THz astronomy. The CAMISTIC project aims to install a filled bolometer-array camera with 16x16 pixels on IRAIT at Dome C and explore the 200-$\mu$m windows for potential ground-based observations.

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