Fig. 12.
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The Robustness of integrated M∗ derived from the spatially resolved SED fitting and the integrated SED fitting compared to the true M∗ from the TNG50 simulation. Left panel: Comparison between M∗ derived from spatially resolved SED fitting (i.e. by summing up M∗ of pixels within the ROI of the galaxies) and the true values. Middle panel: Comparison between M∗ derived from integrated SED fitting and the true values. Right panel: Comparison between integrated M∗ from spatially resolved and integrated SED fitting.
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