  We present a statistical analysis of halo emission for a sample of 1047
edge-on disk galaxies imaged in five bands by the Sloan Digital Sky Survey
(SDSS). Stacking the homogeneously rescaled images of the galaxies, we can
measure surface brightnesses as deep as mu_r~31 mag/arcsec^2. The results
strongly support the almost ubiquitous presence of stellar halos around disk
galaxies, whose spatial distribution is well described by a power-law
$\rho\propto r^{-3}$, in a moderately flattened spheroid (c/a~0.6). The colour
estimates in g-r and r-i, although uncertain, give a clear indication for
extremely red stellar populations, hinting at old ages and/or non-negligible
metal enrichment. These results support the idea of halos being assembled via
early merging of satellite galaxies.
