1.
2. First 450-micron dust continuum mapping of the massive star-forming region NGC 3576 with the P-ArTeMiS bolometer camera;Andre,2008
3. Dubreuil, D. et al, “Optical design for the 450, 350 and 200 μm ArTeMiS camera”, this Proceeding.
4. Reveret, V., “The ArTeMiS wide-field submillimeter camera: on-sky performance at 350 microns”, this Proceeding
5. Use of polypropylene film for infrared cryogenic windows