Fig. 6.
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Stellar population properties derived from the J-spectra (MAG_AUTO) fits with BaySeAGal for the whole miniJPAS sample (grey area and dashed black line), for galaxies in the field (black-line), and galaxies in a group environment (magenta line). From left to right, and from top to bottom: PDF of the galaxy stellar mass, mass-weighted age, stellar extinction, stellar metallicity, rest-frame (u − r) colour, extinction-corrected rest-frame (u − r) colour, and the parameters of the SFH: t0 and τ.
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