Fig. 2.
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SED-fitting analysis (top panel) and residuals (bottom panel) of a miniJPAS galaxy at z = 0.07 (ID 2470-10239). The black dots and vertical bars in the top panel are the galaxy fluxes and errors as observed by miniJPAS, respectively. The red squares are the best-fitting CSP model. The shaded area shows 2.5 times the photon-noise uncertainty of each band.
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