PERFORMANCES OF HERSCHEL/PACS BOLOMETER ARRAYS AND FUTURE DEVELOPMENTS AT CEAPPPP

被引:4
|
作者
Billot, N. [1 ,2 ]
Rodriguez, L. [2 ]
Okumura, K. [2 ]
Sauvage, M. [2 ]
Agnese, P. [3 ]
机构
[1] CALTECH, NASA Herschel Sci Ctr, Ctr Infrared Proc & Anal, MC 100-22, Pasadena, CA 91125 USA
[2] CEA Saclay, IRFU, Serv Astrophys, F-91191 Gif Sur Yvette, France
[3] CEA Grenoble, LETI, Lab Infrarouge, F-38054 Grenoble, France
来源
关键词
MISSION;
D O I
10.1051/eas/0937014
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The European Space Agency is building a space telescope to observe the Universe in the Far-IR and sub-millimeter regime of the electromagnetic spectrum. The scientific payload is composed of three instruments. One of them, PACS, is equipped with a novel type of bolometer arrays developed by CEA in the late 90's. We briefly present the PACS Photometer and the architecture of CEA filled bolometer arrays. We accessed the physics of the detectors and thoroughly measured their performances by developing a pragmatic calibration procedure. The Photometer is now calibrated and integrated on the focal plane of the observatory. The launch is scheduled for April 2009. Meanwhile, CEA is working on adapting PACS bolometers to longer wavelength for wide-field ground-based telescopes, and for the future cold-telescope space mission SPICA.
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收藏
页码:119 / +
页数:2
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