Fig. 1.
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Multipoles of the correlation function (monopole, quadrupole, and hexadecapole from top to bottom) when accounting for RSD only (red), for RSD and lensing magnification (blue), and for RSD and a flat-sky implementation of the lensing magnification. We consider here a ΛCDM model at z = 1.8 with a galaxy bias equal to unity and s = 1.2.
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