Fig. 1
a) (V,Ks) pseudomagnitudes of the 3747 Hipparcos K0 class III and V stars as a function of their distance modulus; b) Absolute (V,Ks) pseudomagnitudes of the same stars, with the dwarfs lying at the top and the giants lying at the bottom of this figure. The decrease of the pseudomagnitudes beyond a certain distance is an artefact due to numerical bias at low signal to noise ratio (see text).
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.