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Review: far-infrared instrumentation and technological development for the next decade

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Academic year: 2021

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Figure

Fig. 1 Atmospheric transmission over 1 to 1000 μm. 71 The curves for ALMA and SOFIA are computed with a 35-deg telescope zenith angle
Table 1 Selected examples of sensitivities achieved by far-infrared to millimeter-wave detector arrays, along with some required for future missions
Fig. 2 (a) The world’s largest flying infrared astronomical observatory, SOFIA (Sec. 2.2)
Fig. 4 The 89 μm image (intensity represented by color) with polari- polari-zation measurements at the same wavelength (black lines), taken using HAWC+ on SOFIA, of ρ-ophiucus (courtesy of Fabio Santos, Northwestern University, Illinois)
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