Individual rest-frame VUDS spectra of the nine zspec members of the z ~ 4.57 proto-structure detected in COSMOS with secure spectroscopic redshifts (see Sect. 2.1.1 for the meaning of this phrase). The spectra were smoothed with a Gaussian filter of σ = 1.5 pixels (~1.5 Å in the rest-frame). The ID of each member galaxy along with its spectroscopic redshift, redshift quality flag, and observed i+ magnitude are shown on the upper left hand corner of each panel. The typical flux density uncertainty as estimated by the NMAD scatter of each spectrum over the wavelengths plotted here is 1.5 × 10−19 ergs s−1 cm−2 Å−1. Colored dotted lines indicate important spectral features. We highlight that in many cases the Lyα emission feature is absent or an identical redshift would have been recovered even in its absence.
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.