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

Open Access

Fig. 1

Star information input maps for a single edge-on galaxy from the NIHAO sample of M_* = 10^10.68 M_⊙. Top: PDF in the ${{\hat{R}}_{proj}, {\hat{v}}_{LOS}}$ $Mathematical equation: $\[\{\hat{R}_{\text {proj}}, \hat{v}_{\text {LOS}}\}\]$$ phase space. Bottom: PDF in the {x,y} phase space. Both obtained following the procedure described in Sect. 3.1.1.

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