Fig. 2.
(J0515 − r) vs. (g − i) color–color diagram from ISO_GAUSS magnitudes of mr ≤ 18 sources with significant J0660 excess. Left panel: sources with no spectroscopic redshift in SDSS. Right panel: J0660 emitters, with spectroscopic redshift in SDSS. Cyan dots represent sources within our redshift of interest, while red dots are sources with higher redshift. The three regions defined to isolate low-z galaxies (R1), blended stars (R2), and high-z galaxies (R3) are labeled in the panel.
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