Spectral energy distribution similarity of the local galaxies and the
  3.6um selected galaxies from the Spitzer Extended Deep Survey
  The Spitzer Extended Deep Survey (SEDS) as a deep and wide mid-infrared (MIR)
survey project provides a sample of 500000+ sources spreading 1.46 square
degree and a depth of 26 AB mag (3$\sigma$). Combining with the previous
available data, we build a PSF-matched multi-wavelength photometry catalog from
u band to 8$\mu$m. We fit the SEDS galaxies spectral energy distributions by
the local galaxy templates. The results show that the SEDS galaxy can be fitted
well, indicating the high redshift galaxy ($z \sim 1$) shares the same
templates with the local galaxies. This study would facilitate the further
study of the galaxy luminosity and high redshift mass function.
