Infrared detector arrays and some applications to spectroscopy

Details Infrared detector arrays and some applications to spectroscopy Infrared detector arrays and some applications to spectroscopy

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.160..333t&link_type=abstract

(Group of Optical and Infrared Astronomers in Japan, Astronomical Society of Japan, Inamori Foundation, et al., International Sy

Astronomy and Astrophysics

Astronomy

1

Astronomical Spectroscopy, Infrared Astronomy, Infrared Detectors, Cryogenic Equipment, Echelle Gratings, Hydroxyl Emission, Thermal Radiation

Scientific paper

The read noise, dark current, and pixel sizes of state-of-the-art infrared arrays for astronomy are presented. Considerations for instrument development utilizing infrared arrays are discussed, with emphasis on the background emission and expected sensitivity. A simple method of estimating the background emission on the JNLT and some applications to spectroscopy are presented.

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