Fig. 3.
Distribution of characteristic parameters of the OTELO [O III] sample. Left: [O III] line flux and observed EW measured in [O III] pseudo-spectra. Line flux and EWobs limits are ∼5 × 10−19 erg s−1 cm−2 and ∼6 Å. Right: morphology and stellar mass distribution of the OTELO [O III] ELS sample. The main morphological classes represented here are: Pl – Point-like; Sph – Spheroid; D – Disk; Tp- Tadpole; Ch – Chain; CC – Clumpy Cluster; Db – Doubles; Unc – Uncertain/Non-classified. At least 127 sources are disc-like galaxies and the median stellar mass is 8.36 × 108 M⊙. See main text for details.
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.