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Fig. 11.


Probability distribution of the median differences in the photometry of MS stars independently observed by two adjacent pointings. In all the panels the black histogram shows the results from the SLR (reference photometry in J-PLUS DR1), the grey filled histogram shows the results after applying Δ𝒳atm, and the coloured histogram after applying Δ𝒳atm and P𝒳 (X, Y). The solid line is the best Gaussian fit to the latest case. The uncertainty in the calibration is labelled in the panels and was estimated as the dispersion of the fitted Gaussian divided by the square root of two. Shown (from top to bottom and left to right) are the filters u, J0378, J0395, J0410, J0430, g, J0515, r, J0660, i, J0861, and z.

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