New WISE W1 color-to-mass-to-light models reproduce Spitzer, S4G and Dustpedia stellar masses, but conflict with the Jarrett et al. GAMA-G23-based calibration by about 0.2 dex.
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The Baryonic Tully-Fisher Relation II: Stellar Mass Models
New WISE W1 color-to-mass-to-light models reproduce Spitzer, S4G and Dustpedia stellar masses, but conflict with the Jarrett et al. GAMA-G23-based calibration by about 0.2 dex.