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-μm windows for potential ground-based observations.
@article{arxiv.astro-ph/0702480,
title = {Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array},
author = {Vincent Minier and Gilles Durand and Pierre-Olivier Lagage and Michel Talvard and Tony Travouillon and Maurizio Busso and Gino Tosti},
journal= {arXiv preprint arXiv:astro-ph/0702480},
year = {2009}
}