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Fig. 14

Fig. 14 Refer to the following caption and surrounding text.

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Same as Fig. 13, except that the TRILEGAL simulation is used instead of Rubin DP1 data. Note: the q = 0.62 and n = 2.75 halo profile assumed in simulations is faithfully reproduced (although it cannot be distinguished from the canonical spherical 1/r3 profile due to sparse coverage of the R–Z plane).

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