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

Vincent Minier·Gilles Durand·Pierre-Olivier Lagage·Michel Talvard·Tony Travouillon·Maurizio Busso·Gino Tosti
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Abstract

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-$μ$m windows for potential ground-based observations.

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Vincent Minier, Gilles Durand, Pierre-Olivier Lagage, Michel Talvard, Tony Travouillon, Maurizio Busso, Gino Tosti. 2007-02-19. Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array. https://doi.org/10.1051/eas%3A2007114

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