Fig. 1.
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Magnitude distribution of the MeerLICHT (ML) q band and the Gaia G band in a field with a galactic latitude above 20° (b = 21.08°), using a magnitude bin width of Δmag = 0.5 mag. The y-axis represents the number of data points per magnitude bin, and the x-axis corresponds to MeerLICHT’s q-band magnitude (qmag) and Gaia G-band magnitude (Gmag). The parallax over parallax error (ϖ/σϖ) and the RUWE cuts are applied independently to the Gaia data. The value in the middle bottom panel corresponds to the median of the RUWE.
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