With the aim of constructing accurate 2D maps of the stellar mass distribution in nearby galaxies from S4G 3.6 and 4.5 µm images, we report on the separation of the light from old stars from the emission contributed by contaminants. Results for a small sample of six disk galaxies (NGC 1566, NG
The mid-infrared is an optimal window to trace stellar mass in nearby galaxies and the 3.6 mm IRAC b...
International audienceThe mid-infrared is an optimal window to trace stellar mass in nearby galaxies...
The mid-infrared is an optimal window to trace stellar mass in nearby galaxies and the 3.6 μ {{m}} I...
With the aim of constructing accurate two-dimensional maps of the stellar mass distribution in nearb...
International audienceWith the aim of constructing accurate two-dimensional maps of the stellar mass...
With the aim of constructing accurate two-dimensional maps of the stellar mass distribution in nearb...
With the aim of constructing accurate two-dimensional maps of the stellar mass distribution in nearb...
We present a new approach for estimating the 3.6 μm stellar mass-to-light ratio Υ3.6 in terms of the...
We present a new approach for estimating the 3.6 mu m stellar mass-to-light (M/L) ratio Rho 3.6 in t...
We present a new approach for estimating the 3.6 μm stellar mass-to-light (M/L) ratio Upsilon3.6 in ...
We present a new approach for estimating the 3.6 μm stellar mass-to-light (M/L) ratio Upsilon3.6 in ...
We present a new approach for estimating the 3.6 mu m stellar mass-to-light (M/L) ratio Rho 3.6 in t...
International audienceWe present a new approach for estimating the 3.6 mu m stellar mass-to-light (M...
The mid-infrared is an optimal window to trace stellar mass in nearby galaxies and the 3.6 μ {{m}} I...
The mid-infrared is an optimal window to trace stellar mass in nearby galaxies and the 3.6 mm IRAC b...
International audienceThe mid-infrared is an optimal window to trace stellar mass in nearby galaxies...
The mid-infrared is an optimal window to trace stellar mass in nearby galaxies and the 3.6 μ {{m}} I...
With the aim of constructing accurate two-dimensional maps of the stellar mass distribution in nearb...
International audienceWith the aim of constructing accurate two-dimensional maps of the stellar mass...
With the aim of constructing accurate two-dimensional maps of the stellar mass distribution in nearb...
With the aim of constructing accurate two-dimensional maps of the stellar mass distribution in nearb...
We present a new approach for estimating the 3.6 μm stellar mass-to-light ratio Υ3.6 in terms of the...
We present a new approach for estimating the 3.6 mu m stellar mass-to-light (M/L) ratio Rho 3.6 in t...
We present a new approach for estimating the 3.6 μm stellar mass-to-light (M/L) ratio Upsilon3.6 in ...
We present a new approach for estimating the 3.6 μm stellar mass-to-light (M/L) ratio Upsilon3.6 in ...
We present a new approach for estimating the 3.6 mu m stellar mass-to-light (M/L) ratio Rho 3.6 in t...
International audienceWe present a new approach for estimating the 3.6 mu m stellar mass-to-light (M...
The mid-infrared is an optimal window to trace stellar mass in nearby galaxies and the 3.6 μ {{m}} I...
The mid-infrared is an optimal window to trace stellar mass in nearby galaxies and the 3.6 mm IRAC b...
International audienceThe mid-infrared is an optimal window to trace stellar mass in nearby galaxies...
The mid-infrared is an optimal window to trace stellar mass in nearby galaxies and the 3.6 μ {{m}} I...