Intrinsic alignments of galaxies in multiple projections

Open Access

Fig. F.2.

Evolution of NLA A_IAb_g when fitting within different scale ranges, shown for particle number and mass cut with upward triangles and solid lines, and downward triangles and dashed lines, respectively. NLA amplitudes fitted with ${\tilde{ξ}}_{g +, 2}$ $\tilde{\xi}_{\mathrm{g+,2}}$ are depicted in dark blue and those fitted with w_g+ in light blue, including the error bars.

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