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Table 1
Color-correction factors (cc) for our bright sources.
| Source | c c 70.0 μm | c c 100.0 μm | c c 160.0 μm | Unc. [%] | Model source |
|
|
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| Mars | 0.947 | 1.033 | 1.054 | ≈1 | mars_esa_2_i.dat (Moreno) |
| Uranus | 0.984 | 0.995 | 1.018 | ≈1 | orton_uranus_esa5 (Orton) |
| Uranus | 0.984 | 0.992 | 1.019 | ≈1 | ura_esa2_2_i.dat (Moreno) |
| Neptune | 0.984 | 0.993 | 1.020 | ≈1 | nep_esa5_2_i.dat (Moreno) |
| Callisto | 0.998 | 1.016 | 1.055 | ≈1 | call_esa2_2_i.dat (Moreno) |
| Ganymede | 0.996 | 1.014 | 1.053 | ≈1 | gany_esa2_2_i.dat (Moreno) |
| Titan | 0.985 | 1.002 | 1.028 | ≈2 | tit_esa3_2_i.dat (Moreno) |
| fiducial stars | 1.016 | 1.033 | 1.074 | ≈1 | Balog et al. (2014) |
Notes. Models are taken from ftp://ftp.sciops.esa.int/planets/originalData/. The estimated maximal uncertainty for these corrections is 2% for Titan and about 1% for the rest of the targets.
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