Fig. 13


Observed star formation rate surface density, ΣSFR, measured using the effective radius in kiloparsecs as measured in JF125W (van der Wel et al. 2014) (color coding) vs. C III] EW for galaxies in the udf-10 . At these redshifts, the JF125W band covers the rest-frame optical region of the galaxy SED probing the stellar continuum, whereas the C III] comes from the UV-dominated star-forming regions. The HDFS region is not covered with HST imaging at these wavelengths. The results are consistent when using the HF160W sizes. Only the two largest galaxies here are resolved at the spatial resolution with MUSE.

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