Stellar mass-to-light ratios for nearby galaxies are most stable near 1.6 microns, and correcting for star formation rate reduces the scatter to about 0.02 dex.
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Accuracy of Stellar Mass-to-light Ratios of Nearby Galaxies in the Near-Infrared
Stellar mass-to-light ratios for nearby galaxies are most stable near 1.6 microns, and correcting for star formation rate reduces the scatter to about 0.02 dex.