Fig. 5
Nine nearest healpixels toward a single Taurus-Perseus position (here, L1544). Each column corresponds to a wavelength. The top row shows the DIRBE values (rescaled to 2MASS or Spitzer units), the middle row the star flux contribution (PSC), and the bottom row the remaining diffuse emission Idiff(λ). Gray scale and values are given in MJy sr-1.
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