Fig. 2.

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Photo-spectra of the miniJPAS sources classified as H-dominated DAs in descending effective temperature from the top-left to bottom-right corner. Colored circles represent the 56 medium bands, and squares indicate the g and i broadbands. The presented fluxes were estimated from the 3 arcsec diameter aperture photometry corrected for aperture effects (Sect. 2.2), and no correction for interstellar reddening was applied. The gray diamonds show the theoretical flux from the best-fitting model to the data. The parameters of the fitting are labeled in the panels. The solid brown line depicts the SDSS spectra of the sources with a downgraded resolution of R ∼ 90 for a better comparison. The flux of the SDSS spectra were scaled to match the miniJPAS r-band photometry. The flux scale of the SDSS spectra for the sources 2243–2625, 2406–5601, and 2406–16326 has an additional factor (λ/λ0)a applied, with λ0 = 6254 Å and a = 1.1, 0.3, and −0.4, respectively.
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