Fig. 6


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.

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