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- W2012364245 abstract "The infrared sky from space is the sum of a cosmic signal from galaxies, quasars, and perhaps more exotic sources; and foregrounds from the Milky Way and from the Solar System. At a distance of 1 AU from the Sun, the foreground from interplanetary dust is very bright between 5 and 100 μm, but “very bright” is still several million times fainter than the background produced by ground-based telescopes. In the near infrared 1–2.2 μm range the space infrared sky is a thousand times fainter than the OH nightglow from the Earth’s atmosphere. As a result of these advantages, wide-field imaging from space in the infrared can be an incredibly sensitive method to study the Universe." @default.
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- W2012364245 date "2005-11-01" @default.
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- W2012364245 title "The infrared sky" @default.
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- W2012364245 doi "https://doi.org/10.1016/j.newar.2005.08.013" @default.
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