Comparison of the ﹩A_{V}﹩ map derived from high‐﹩T_{E}﹩ stars (smoothed to match the IRAS spatial resolution), an IRAS 100 μm image (log scaled), and a stellar density image of main‐sequence stars with ﹩V< 16.5﹩ and B−﹩V< 0.5﹩. The vertical bar at the right of the upper panel indicates the scan that has nonphotometric I‐band data.