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Strong Clustering of Lyman Break Galaxies around Luminous Quasars at Z ∼ 4

  • Authors: Cristina García-Vergara, Joseph F. Hennawi, L. Felipe Barrientos, and Hans-Walter Rix

2017 The Astrophysical Journal 848 7.

  • Provider: AAS Journals

Caption: Figure 14.

QSO–LBG cross-correlation function and its maximum likelihood model. The filled circles show our measurement described in Section 4.1 with ﹩1\sigma ﹩ Poisson error bars. The solid red curve shows the best maximum likelihood estimator for both rQG0 and γ as free parameters. We obtain ﹩{r}_{0}^{\mathrm{QG}}\,=6.93\,{h}^{-1}\,\mathrm{cMpc}﹩ and ﹩\gamma =2.4﹩. The dashed black line shows the theoretical expectation of ﹩\chi ({R}_{\min },{R}_{\max })﹩ for the six stacked fields calculated from the independently determined QSO and LBG auto-correlation functions, assuming a deterministic bias model.

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