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

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Fig. 2

Gas information input maps for a single galaxy from the NIHAO sample of M_* = 10^10.68 M_⊙ at increasing inclinations from edge-on to 60 degrees. From left to right: HI intensity, average line-of-sight velocity, and velocity dispersion maps, obtained following the procedure described in Sect. 3.1.2.

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