Volume-averaged two-point correlation functions as a function of the B absolute luminosity (upper panels) and stellar mass (lower panels). The limits of the subsamples in absolute magnitude and stellar mass are shown in the left upper and lower panels. Black triangles: M_B(z = 1.1) − 5log (h) ≤ −19.5 (log (M_∗/M_⊙h^-2 ≥ 9.0 M_⊙); red squares: M_B(z = 1.1) − 5log (h) ≤ −20.0 (log (M_∗/M_⊙h^-2 ≥ 9.5 M_⊙); blue pentagons: M_B(z = 1.1) − 5log  (h) ≤ −20.5 (log (M_∗/M_⊙h^-2 ≥ 10.0 M_⊙); green hexagons: M_B(z = 1.1) − 5log (h) ≤ −21.0 (log (M_∗/M_⊙h^-2 ≥ 10.5 M_⊙); magenta heptagons: M_B(z = 1.1) − 5log  (h) ≤ −21.5 (log (M_∗/M_⊙h^-2 ≥ 11.0 M_⊙). Dotted lines: real-space for the M_B(z = 1.1) − 5log  (h) ≤ −20.5 (log (M_∗/M_⊙h^-2 ≥ 10.0 M_⊙) subsamples in the redshift bin [0.5, 0.7], predicted from the power-law fit of ξ₂ in Marulli et al. (2013).