A liquid helium cooled mid-infrared imaging Fabry-Perot spectrometer

Details A liquid helium cooled mid-infrared imaging Fabry-Perot spectrometer A liquid helium cooled mid-infrared imaging Fabry-Perot spectrometer

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994exa.....3..179w&link_type=abstract

Experimental Astronomy, vol. 3, no. 1-4, p. 179-180

Astronomy and Astrophysics

Astronomy

Arrays, Astronomical Spectroscopy, Fabry-Perot Spectrometers, Infrared Detectors, Infrared Spectrometers, Doped Crystals, Infrared Astronomy, Phosphorus, Silicon

Scientific paper

A liquid helium cooled mid-infrared imaging Fabry-Perot spectrometer has been under development. A Si:P 5x5 detector array is used for this instrument. Although the array system has small format, but combination with junction field effect transistor (JFET) array will provide noise equivalent line flux of 1.0 x 10-21 w/sq cm(1000 sec, 10 sigma). This sensitivity is comparable with the short wavelength spectrometer (SWS) of the Infrared Space Observatory (ISO).

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