Infrared astronomy on the Hubble Space Telescope |
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Authors: | J.L. Pipher S.P. Willner G.G. Fazio |
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Affiliation: | 1. Phys. and Astron. Dept., University of Rochester, Rochester, NY 14627, U.S.A.;2. Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, U.S.A. |
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Abstract: | ![]() The Hubble Space Telescope offers enormous advantages to infrared astronomy in certain situations. The advantages of being above the atmosphere include an increase in spatial resolution, a much wider range of wavelengths available, and lower background radiation. Compared to proposed cooled telescopes, HST offers higher spatial resolution and increased collecting area. HST is particularly well suited to observations at wavelengths less than ~5 μm, where the diffraction limit is less than the seeing limit from the ground and thermal emission does not seriously compromise the sensitivity of the detectors. HST is also favorable for observations requiring high spectral resolution at all wavelengths not accessible from the ground. |
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