Table 2
Top part of the table: slopes and respective errors computed for our three spectra and for the spectrum of Makemake from Licandro et al. (2006b). Bottom part: slopes and respective errors calculated for the spectrum of Eris from (a) Alvarez-Candal et al. (2011) and for the spectrum of Pluto from (b) Pinilla-Alonso (priv. comm.).
| Data | Slope (0.40−0.52 μm) | Error |
|
|
||
| Phase 1 | 23%/1000 Å | 4%/1000 Å |
| Phase 2 | 20%/1000 Å | 4%/1000 Å |
| Phase 3 | 32%/1000 Å | 4%/1000 Å |
| Licandro et al. (2006b) | 26%/1000 Å | 4%/1000 Å |
|
|
||
| Erisa | 12%/1000 Å | 4%/1000 Å |
| Plutob | 28%/1000 Å | 4%/1000 Å |
Notes. All the slopes were computed between 0.40−0.52 μm and for spectra normalized at 0.55 μm.
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