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Fig. 1.

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Stellar number density distribution for a few area cells of the data sample with 2 < MG ≤ 3. Each panel is labelled by the area cell’s mid-point (X, Y) coordinates. The function obtained by GP regression is shown in solid black; the fitted symmetric function ( n ̂ $ \hat{n} $) of Eq. (5) is shown in dashed red; the raw number count (N) with its associated Poisson noise uncertainty is shown as a 1σ band.

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