  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.
