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Fig. 11.

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Metallicity difference between J-PLUS photometric values and APOGEE spectroscopic values, Δ[Fe/H], as a function of Galactic latitude b. Left panel: using 𝒳ISL photometry. Right panel: using 𝒳ISL + ZSL photometry. The solid lines in both panels show the best linear fitting to the data, with the gray areas depicting the 68% and 95% confidence intervals. The dashed lines mark zero difference. The dotted line in the right panel shows a difference of 0.02 dex.

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