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Bolometers at CEA: ARTEMIS and beyond

  • P. Kern, V. Revéret (a1), M. Talvard (a1), P. André (a1), L. Rodriguez (a1), Y. Le-Pennec (a1), C. De Breuck (a2), P. Agnèse (a3), O. Boulade (a1), C. Delisle (a1), E. Doumayrou (a1), D. Dubreuil (a1), E. Ercolani (a4), P. Gallais (a1), B. Horeau (a1), P.-O. Lagage (a1), B. Leriche (a5), M. Lortholary (a1), J. Martignac (a1), V. Minier (a1), E. Pantin (a1), D. Rabanus (a6), J. Relland (a7), F. Visticot (a1) and G. Willmann (a8)...

Abstract

ArTeMiS is a bolometer camera that will be installed at the APEX submillimeter telescope in Chile in 2010. This instrument will be a powerful tool for scientists with its three focal planes that will operate simultaneously in background limited conditions at 200, 350 and 450 microns (5760 pixels in total). A prototype called p-ArTeMiS has been tested at APEX in 2007 and thanks to its good performances, the team has been able to conduct scientific projects in star formation and on debris disks. This paper summarises the details of the ArTeMiS project, with a description of the detectors, the optics, the cryogenics and the electronics. We will also present the undergoing studies at CEA on detectors for the future submillimeter space missions.

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[1] André, P., et al., 2008, A&A, 490, L27
[2] Billot, N., et al., 2006, Proc. SPIE, 6265, 62650D
[3] Minier, V., et al., 2009, A&A, to be published
[4] Revéret, V., et al., 2008, J. Low Temp. Phys., 151, 1
[5] Swinyard, B., 2008, 37th COSPAR Scient. Assembly, 3104
[6] Talvard, M., et al., 2008, Proc. SPIE, 7020, 70200A

Bolometers at CEA: ARTEMIS and beyond

  • P. Kern, V. Revéret (a1), M. Talvard (a1), P. André (a1), L. Rodriguez (a1), Y. Le-Pennec (a1), C. De Breuck (a2), P. Agnèse (a3), O. Boulade (a1), C. Delisle (a1), E. Doumayrou (a1), D. Dubreuil (a1), E. Ercolani (a4), P. Gallais (a1), B. Horeau (a1), P.-O. Lagage (a1), B. Leriche (a5), M. Lortholary (a1), J. Martignac (a1), V. Minier (a1), E. Pantin (a1), D. Rabanus (a6), J. Relland (a7), F. Visticot (a1) and G. Willmann (a8)...

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