Fig. 11.
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CR7 properties derived from the emission line and SED fitting of the low-resolution data cube. From left to right, the surface SFR density derived from the Hα spatially resolved emission (see Eq. (3.6.1)) and the SFR within the past 10 Myr and 100 Myr derived with prospector are shown (see Sect. 3.6). Black contours are arbitrary [O III]λ5007 flux levels.
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