Highlight
Free Access

Fig. 3

thumbnail

Stellar number density computed from the evolution tracks assuming only IMF (a), top) and IMF+SFR (b), bottom) without colour cuts. Middle panels: with the colour cut (0.23 <JK< 0.45) and stellar parameter limits (3.5 ≤ log g ≤ 4.5) to simulate the selection effect of the survey and our stellar sample. Right: the suppression factor, defined as the ratio of stars with cut to the number of stars without cut, i.e. the larger the number the more stars are suppressed (see text).

This figure is made of several images, please see below:

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.