Fig. 1.

Diagnostic diagram WHAN (Cid Fernandes et al. 2011) to distinguish star formation-dominated galaxies from AGNs for the LoCuSS mass-complete cluster and field galaxy samples. The star-forming region of the WHAN diagram is populated by 410 cluster galaxies and 227 field galaxies (SFgals sample, red, green, and cyan points) with rest-frames EW(Hα) > 3 Å and log([NII]/Hα)≤ − 0.3. The red symbols show the subsample of SFgals with R < R200. Mlow (Mhigh) galaxies shown as black symbols in the lower (upper) panels lie in the region occupied by Type-2 AGNs (SeyfLiners sample, see Table 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.