  We present an initial analysis of the properties of the all-sky image
obtained by the Far-Infrared Surveyor (FIS) onboard the AKARI satellite, at
65~$\mu$m (N60), 90~$\mu$m (WIDE-S), 140~$\mu$m (WIDE-L),and 160~$\mu$m (N160).
Absolute flux calibration was determined by comparing the data with the
COBE/DIRBE data sets, and the intensity range was as wide as from a few
MJy~sr$^{-1}$ to $>$1~GJy~sr$^{-1}$. The uncertainties are considered to be the
standard deviations with respect to the DIRBE data, and they are less than 10\%
for intensities above 10, 3, 25, and 26~MJy~sr$^{-1}$ at the N60, WIDE-S,
WIDE-L, and N160 bands, respectively. The characteristics of point sources in
the image were also determined by stacking maps centred on photometric standard
stars. The full width at half maxima of the point spread functions (PSFs) were
63$"$, 78$"$, and 88$"$ at the N60, WIDE-S, and WIDE-L bands, respectively. The
PSF at the N160 band was not obtained due to the sensitivity, but it is thought
to be the same as that of the WIDE-L one.
