Fig. B.1.
Download original image
Comparison of Gaia DR3 Apsis GSP-Phot distances with asteroseismic values computed using E20 and APOGEE for Kepler (left), K2 (middle), and TESS (right). The bottom panels show the relative difference in distance. The colour scale indicates the Gaia parallax-to-error ratio. See Fig. 9 in Fouesneau et al. (2023) for a similar comparison with other asteroseismic datasets.
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.