Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-27T10:17:06.988Z Has data issue: false hasContentIssue false
  • English
  • Français

CEA development of filled bolometer arrays at submillimeter wavelengthsA possible application to ground-based telescopes at Dome C

Published online by Cambridge University Press:  05 January 2006

M. Giard ,
F. Casoli ,
F. Paletou ,
V. Minier ,
V. Revéret ,
L. Rodriguez ,
J. Le Pennec ,
P. André ,
B. Horeau  and
P. Agnèse
V. Minier
Affiliation:
Service d'Astrophysique/DAPNIA/DSM/CEA CE de Saclay, 91191 Gif-sur-Yvette, France
V. Revéret
Affiliation:
Service d'Astrophysique/DAPNIA/DSM/CEA CE de Saclay, 91191 Gif-sur-Yvette, France European Southern Observatory, Alonso de Cordova 3107, Vitacura, Santiago, Chile
L. Rodriguez
Affiliation:
Service d'Astrophysique/DAPNIA/DSM/CEA CE de Saclay, 91191 Gif-sur-Yvette, France
J. Le Pennec
Affiliation:
Service d'Astrophysique/DAPNIA/DSM/CEA CE de Saclay, 91191 Gif-sur-Yvette, France
P. André
Affiliation:
Service d'Astrophysique/DAPNIA/DSM/CEA CE de Saclay, 91191 Gif-sur-Yvette, France
B. Horeau
Affiliation:
Service d'Astrophysique/DAPNIA/DSM/CEA CE de Saclay, 91191 Gif-sur-Yvette, France
P. Agnèse
Affiliation:
Laboratoire InfraRouge/LETI/CEA CE de Grenoble, 17 avenue des Martyrs, 38054 Grenoble, France
Get access

Abstract

Accompanying the development of the PACS photometer camera (60–210 μm)on the Herschel Space Observatory, CEA/SAp and CEA/LETI have developed anew type of filled bolometer arrays. We present a camera using these “CCD-like”detectors for ground-based submillimeter applications. Such an instrument could potentially be operated in all atmospheric windows between 200 and 870 μmon a submillimetre-wave single-dish telescope at Dome C. A bolometer arraycould consist of several monolithic units of 16 × 16 pixels (as an example the blue and red PACS arrays consist of 4 × 2 and 2 × 1 units,respectively), providing a full sampling of the focal plane.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 14: Dome C Astronomy and Astrophysics Meeting , 2005 , pp. 343 - 348
Copyright
© EAS, EDP Sciences, 2005

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)