Nifte: The near infrared faint-object te
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James J. Bock; Andrew E. Lange; T. Matsumoto; Peter B. Eisenhardt; Perry B. Hack
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Article
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1994
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Springer
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English
โ 139 KB
The high sensitivity of large format InSb arrays can be used to obtain deep images of the sky at 3-5 pm. In this spectral range cool or highly redshifted objects (e.g. brown dwarfs' and protogalaxies) which are not visible at shorter wavelengths may be observed. Sensitivity at these wavelengths in g