Gaia Data Release 3 - Astrometric orbit determination with Markov chain Monte Carlo and genetic algorithms: Systems with stellar, sub-stellar, and planetary mass companions

Open Access

Fig. 7.

Parameter distributions of the published solutions: Period-eccentricity and period vs. semi-major axis (top panels), apparent magnitude vs. inverse parallax (third panel), and zero-extinction absolute magnitude vs. colour (bottom panel). See Sects. 6.1.4 and 6.2 for a discussion.

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.