Fig. 8
Redshift-space 2PCF of VIPERS galaxies compared to theoretical expectations as a function of B-band magnitude (upper panels) and stellar mass (bottom panels). The coloured symbols used for VIPERS measurements are the same as in Fig. 3. The grey shaded areas show the 2PCF measured in two large galaxy mock catalogues, constructed with the Munich semi-analytic model. The 2PCFs in different sub-samples are offset by 0.5 dex, starting from the lower luminosity and stellar mass samples, for visual clarity.
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