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Fig. 1.
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M − λ relation of halos in the Magneticum 5 × 5 deg2 light cone, given a galaxy selection of M★ ≥ 109.8 M⊙, mean stellar age ≥ 4.2 Gyr, sSFR ≤ 10−15 yr−1, and cylindrical depth of 60 h−1 cMpc. The relation fit to λ ≥ 5 (dashed line) is consistent with DES-Y1 results within 1σ (To et al. 2021a, blue line and shaded region).
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