Fig. 6

image

HST WFC3/G141 grism spectra (~1.11.7 μm) for all C III] emitters in the MUSE udf-10 region. For each object we show (top) the stacked two-dimensional grism spectrum and (bottom) the individual one-dimensional optimally extracted data points for each grism frame with the median and best-fit model shown in pink. The vertical lines denote the positions of [O II], Hβ, [O III], and Hα based on the MUSE redshift, with >3σ detections in black and nondetections in red. All objects in this area with a rest-frame [O III] EW in excess of 250 Å, the so-called extreme emission line galaxies (Maseda et al. 2014), are C III] emitters.

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.