Constraints on the Dark Side of the Universe and Observational Hubble Parameter Data
Figure 1
Detection of radial (-direction) BAO by [64, Figure 13] in the full LRG sample. This is the correlation pattern along the -direction and should not be confused with the monopole pattern in Figure 3 of [63]. The effect of weak lensing magnification can bee seen by comparing the solid and short dashed curves, which shows that the magnification systematically moves the peak location towards the higher scales. The dash-dotted (blue) curve shows the range by allowing the fiducial distance-redshift relation used in the analysis to vary in a parameterized way, accounting for the systematic error introduced by the mere using of a fiducial model.
