Fig. 32

image

Residuals from a global GGRP = f(GBPGRP) relation for asample of luminous, low extinction stars (A0 < 0.05 mag, MG < 4 mag). Top: as a function of G, colour-coded by the number of stars normalised by the total number of stars per magnitude bin. Bottom: as a function of GBPGRP for a sample of bluer stars, colour-coded by the magnitude.

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.