Fig. 7.
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Clustering length r0 as a function of stellar mass. The GAEA predictions for the PMS at different redshifts are marked by different colours and linetypes (see legend). The data compilation is from Meneux et al. (2008, triangles), Foucaud et al. (2010, stars), Wake et al. (2011, hexagons), Lin et al. (2012, squares), Marulli et al. (2013, diamonds), Durkalec et al. (2018, circles).
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