𝔖 Bobbio Scriptorium
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Faint Star Counts in the Near‐Infrared

✍ Scribed by Hutchings, J. B.; Stetson, P. B.; Robin, A.; Webb, T.

Book ID
123914119
Publisher
University of Chicago Press
Year
2002
Tongue
English
Weight
193 KB
Volume
114
Category
Article
ISSN
0004-6280

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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