Table 1
Jupiter phase curves’ preferred models.
| Wavelength [nm] | Filter | Preferred model | Weight |
|---|---|---|---|
| 260 | UV1 | CB | 1.00 |
| 460 | BL1 | CB | 0.99 |
| 570 | GRN | CB | 1.00 |
| 650 | RED | CB | 1.00 |
| 730 | MT2 | CB | 1.00 |
| 750 | CB2 | CB | 1.00 |
| 890 | MT3 | SH | 1.00 |
| 940 | CB3 | CB | 1.00 |
Notes. For each of Jupiter’s Cassini phase curves we report here the preferred model from our fitting procedure. 7/8 phase curves prefer the coherent backscattering model (CB) over the shadow hiding model (SH). The wavelength column refers to the effective wavelength of the filter used. ‘Weight’ is the LOO model weight of the preferred model.
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