Give to Ursa Minor what is Ursa Minor’s: An updated census of the RR Lyrae population in the Ursa Minor dwarf galaxy based on Gaia DR3

Open Access

Fig. B.5

Same as in Fig. B.4 but for the confirmed RR Lyrae star V134 and the candidate RR Lyrae V156. The periods adopted to fold the light curves are those determined in this work using the Gaia DR3 G-band time series data (see Sec. 5.2).

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.