Share Email Print
cover

Proceedings Paper

Development of stressed Ge:Ga 2D array
Author(s): Shin'ichiro Makiuti; Yasuo Doi; Hiroshi Shibai; Norihisa Hiromoto; Takao Nakagawa; Mitsunobu Kawada; Kenichi Okumura; Haruyuki Okuda
Format Member Price Non-Member Price
PDF $17.00 $21.00

Paper Abstract

We are developing a stressed Ge:Ga 2D array detector that will be used for balloon-borne and satellite-born astronomical observations at wavelength between 100 and 200 micrometers . We have succeeded in making a 4 X 8 element stressed array detector with a stress of 600 N/mm2 and responsivity peak wavelength moved to about 165 micrometers . This has the largest number of pixels at the present time. The responsivities of the detector are high enough as well as those currently in use. This detector has a compact structure and a small total pixel size, and thus, it can be used for satellite-born instruments that have severe space limitation.

Paper Details

Date Published: 21 August 1998
PDF: 8 pages
Proc. SPIE 3354, Infrared Astronomical Instrumentation, (21 August 1998); doi: 10.1117/12.317308
Show Author Affiliations
Shin'ichiro Makiuti, Institute of Space and Astronautical Science (Japan)
Yasuo Doi, Univ. of Tokyo (Japan)
Hiroshi Shibai, Nagoya Univ. (Japan)
Norihisa Hiromoto, Communications Research Lab. (Japan)
Takao Nakagawa, Institute of Space and Astronautical Science (Japan)
Mitsunobu Kawada, Institute of Space and Astronautical Science (Japan)
Kenichi Okumura, Communications Research Lab. (Japan)
Haruyuki Okuda, Institute of Space and Astronautical Science (Japan)


Published in SPIE Proceedings Vol. 3354:
Infrared Astronomical Instrumentation
Albert M. Fowler, Editor(s)

© SPIE. Terms of Use
Back to Top