Beyond single tracers: Convolutional neural network-based inference of galaxy mass profiles from combined gas and stellar kinematics

Open Access

Fig. 6

Ratio of the mass predicted by the neural network models to the real mass enclosed within different radii of the galaxies in the test sets of NIHAO galaxy projections. Shown are the results for the StarGas model applied to two subsets of galaxies with M_* < 10^9.5 M_⊙ and M_* > 10^9.5 M_⊙.

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