  We present the properties of 11 $\mu$m selected sources detected in the early
data of the North Ecliptic Pole Deep (NEP-Deep) Survey of AKARI. The data set
covers 6 wavelength bands from 2.5 to 11 $\mu$m, with the exposure time of 10 ~
20 minutes. This field lies within the CFHT survey with four filter bands ($g',
r', i',z'), enabling us to establish nearly continuous spectral energy
distributions (SEDs) for wavelengths ranging from 0.4 to 11 $\mu$m. The main
sample studied here consists of 71 sources whose 11 $\mu$m AB magnitudes are
equal to or brighter than 18.5 (251 $\mu$Jy), which is complete to more than
90%. The 11 $\mu$m band has an advantage of sampling star forming galaxies with
low to medium redshifts since the prominent PAH feature shifts into this band.
As expected, we find that the majority (~68%) of 11 $\mu$m bright sources are
star forming galaxies at 0.2 < z < 0.7 with $L_{IR} ~ 10^{10}$ -- $10^{12}
L_{\odot}$ based on the detailed modelling of SEDs. We also find four AGNs
lying at various redshifts in the main sample. In addition, we discuss a few
sources which have non-typical SEDs of the main sample, including a brown dwarf
candidate, a steep power-law source, flat spectrum object, and an early-type
galaxy at moderate redshift.
