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Proceedings Paper

The CRIRES InSb megapixel focal plane array detector mosaic
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Paper Abstract

For the high-resolution IR Echelle Spectrometer CRIRES (1-5 μm range), to be installed at the VLT in 2005, ESO is developing a 512 x 4096 pixels focal plane array mosaic based on Raytheon Aladdin III InSb detectors with a cutoff wavelength of 5.2 microns. To fill the useful field of 135 mm in the dispersion direction and 21 mm in the spatial direction and to maximize simultaneous spectral coverage, a mosaic solution similar to CCD mosaics has been chosen. It allows a minimum spacing between the detectors of 264 pixels. ESO developed a 3-side buttable mosaic package for both the Aladdin II and Aladdin III detectors which are mounted on multilayer co-fired AlN ceramic chip carriers. This paper presents the design of the CRIRES 512 x 4096 pixel Aladdin InSb focal plane array and a new test facility for testing mosaic focal planes under low flux conditions.

Paper Details

Date Published: 29 September 2004
PDF: 8 pages
Proc. SPIE 5499, Optical and Infrared Detectors for Astronomy, (29 September 2004); doi: 10.1117/12.551501
Show Author Affiliations
Reinhold J. Dorn, European Southern Observatory (Germany)
Gert Finger, European Southern Observatory (Germany)
Gotthard Huster, European Southern Observatory (Germany)
Hans-Ulrich Kaeufl, European Southern Observatory (Germany)
Jean-Louis Lizon, European Southern Observatory (Germany)
Leander Mehrgan, European Southern Observatory (Germany)
Manfred Meyer, European Southern Observatory (Germany)
Jean-Francois Pirard, European Southern Observatory (Germany)
Armin Silber, European Southern Observatory (Germany)
Joerg Stegmeier, European Southern Observatory (Germany)
Alan F. M. Moorwood, European Southern Observatory (Germany)


Published in SPIE Proceedings Vol. 5499:
Optical and Infrared Detectors for Astronomy
James D. Garnett; James W. Beletic, Editor(s)

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