Free Access
Table 6
Differences in the log evidence of each model relative to the best GP noise model for targets with measured stellar rotation period.
| Model | HD 49933 IRa01 | HD 49933 LRa01 | HD 52265 | HD 179079 |
|---|---|---|---|---|
| G1 | −6776 | −18489 | −11223 | −1768 |
| G2 | −786 | −2270 | −1514 | −222 |
| G3 | −161 | −478 | −344 | −130 |
| G4 | −125 | −240 | −152 | −17 |
| G5 | −112 | −211 | −144 | −18 |
| G1R1 | −251 | −574 | −845 | −125 |
| G2R1 | −121 | −188 | −137 | −18 |
| G3R1 | −112 | −181 | −136 | −13 |
| G2R1O1 | 0 | 0 | 0 | 0 |
| G3O1 | −9 | −84 | −56 | −6 |
| G4O1 | − | − | −16 | − |
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.