Table 2
Considered observing wavelengths.
| λ[μm] | Instrument |
|---|---|
| 10.5 | e.g., VLT/VISIR (a) |
| 24 | Spitzer (b)/MIPS (c) |
| 70 | Spitzer/MIPS, Herschel (d)/PACS (e) |
| 100 | Herschel/PACS |
| 160 | Spitzer/MIPS, Herschel/PACS |
| 214 | SOFIA (f)/HAWC+ (g) |
| 450 | JCMT/SCUBA2 (h), ALMA (i) |
| 850 | JCMT/SCUBA2, ALMA |
| 1300 | ALMA |
Notes. Typical wavelengths and corresponding astronomical instruments for existing debris disk observations.
References. (a)Lagage et al. (2004); (b)Werner et al. (2004); (c)Rieke et al. (2004); (d)Pilbratt et al. (2010); (e)Poglitsch et al. (2010); (f)Temi et al. (2018); (g)Harper et al. (2018); (h)Holland et al. (2013); (i)Kurz et al. (2002).
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