The Antarctic Planet Interferometer (2008)
Swain, Mark R., Walker, Christopher K., Traub, Wesley A., Storey, John W., Coude Du Foresto, Vincent, Fossat, Eric, ...
The Antarctic Planet Interferometer is an instrument concept designed to detect and characterize extrasolar planets by exploiting the unique potential of the best accessible site on earth for thermal...
Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array (2007)
Minier, Vincent, Durand, Gilles, Lagage, Pierre-Olivier, Talvard, Michel, Travouillon, Tony, Busso, Maurizio, ...
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...
Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array (2007)
Minier, Vincent, Durand, Gilles, Lagage, Pierre-Olivier, Talvard, Michel, Travouillon, Tony, Busso, Maurizio, ...
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...
Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array (2007)
Minier, Vincent, Durand, Gilles, Lagage, Pierre-Olivier, Talvard, Michel, Travouillon, Tony, Busso, Maurizio, ...
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...
A search for propylene oxide and glycine in Sagittarius B2 (LMH) and Orion (2007)
Cunningham, Maria R., Jones, Paul A., Godfrey, Peter D., Cragg, Dinah M., Bains, Indra, Burton, Michael G., ...
We have used the Mopra Telescope to search for glycine and the simple chiral molecule propylene oxide in the Sgr B2 (LMH) and Orion KL, in the 3-mm band. We have not detected either species, but have...
A search for propylene oxide and glycine in Sagittarius B2 (LMH) and Orion (2007)
Cunningham, Maria R., Jones, Paul A., Godfrey, Peter D., Cragg, Dinah M., Bains, Indra, Burton, Michael G., ...
We have used the Mopra Telescope to search for glycine and the simple chiral molecule propylene oxide in the Sgr B2 (LMH) and Orion KL, in the 3-mm band. We have not detected either species, but have...
A search for propylene oxide and glycine in Sagittarius B2 (LMH) and Orion (2007)
Cunningham, Maria R., Jones, Paul A., Godfrey, Peter D., Cragg, Dinah M., Bains, Indra, Burton, Michael G., ...
We have used the Mopra Telescope to search for glycine and the simple chiral molecule propylene oxide in the Sgr B2 (LMH) and Orion KL, in the 3-mm band. We have not detected either species, but have...
A search for propylene oxide and glycine in Sagittarius B2 (LMH) and Orion (2007)
Cunningham, Maria R., Jones, Paul A., Godfrey, Peter D., Cragg, Dinah M., Bains, Indra, Burton, Michael G., ...
We have used the Mopra Telescope to search for glycine and the simple chiral molecule propylene oxide in the Sgr B2 (LMH) and Orion KL, in the 3-mm band. We have not detected either species, but have...
Site testing in summer at Dome C, Antarctica (2005)
Aristidi, Eric, Agabi, Abdelkrim, Fossat, Eric, Azouit, Max, Martin, Francois, Sadibekova, Tatiana, ...
We present summer site testing results based on DIMM data obtained at Dome C, Antarctica. These data have been collected on the bright star Canopus during two 3-months summer campaigns in 2003-2004...
Site testing in summer at Dome C, Antarctica (2005)
Aristidi, Eric, Agabi, Abdelkrim, Fossat, Eric, Azouit, Max, Martin, Francois, Sadibekova, Tatiana, ...
We present summer site testing results based on DIMM data obtained at Dome C, Antarctica. These data have been collected on the bright star Canopus during two 3-months summer campaigns in 2003-2004...
Site testing in summer at Dome C, Antarctica (2005)
Aristidi, Eric, Agabi, Abdelkrim, Fossat, Eric, Azouit, Max, Martin, Francois, Sadibekova, Tatiana, ...
We present summer site testing results based on DIMM data obtained at Dome C, Antarctica. These data have been collected on the bright star Canopus during two 3-months summer campaigns in 2003-2004...