Fig. 4.
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Diagram showing the effective radius as a function of r magnitude, used to select candidates to be EELGs for those objects with excess flux in J0515 and no data in the unWISE catalog (grey dots). All sources with SDSS spectra are shown in colors. The color code for those is the same as the one used in Fig. 2, but in this case objects with W1 data are shown in a lighter shade.
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