The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at $0.5 < z < 1.1$
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![Fig. 8. Constraints on b 1 and b 2 from the log(M/M ⊙ ]) > 9 sam- sam-ple, at scales r 12 = 10 h − 1 Mpc and r 13 = 20 h − 1 Mpc](https://thumb-eu.123doks.com/thumbv2/123doknet/13041317.382435/9.892.473.818.86.445/fig-constraints-log-sam-sam-scales-mpc-mpc.webp)
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