Now showing items 1-1 of 1
Reconstructing the stellar mass distributions of galaxies using S 4G IRAC 3.6 and 4.5 μm images. II. the conversion from light to mass
We present a new approach for estimating the 3.6 μm stellar mass-to- light (M/L) ratio Υ3.6 in terms of the [3.6]-[4.5] colors of old stellar populations. Our approach avoids several of the largest sources of uncertainty ...