  The first results of an observational programme aimed at mapping a sample of
face--on spiral galaxies in the NIR are presented. This paper shows the surface
photometry of the first ten galaxies in the sample. The data were taken in the
broad band $J$ (1.2 $\mu$m) and $K_{s}$ (2.2 $\mu$m) filters. The sources were
selected mainly according to their size and brightness in order to suit the
characteristics of the CAIN 2D NIR camera on the 1.5 m Carlos S\'anchez
Telescope (Tenerife, Spain). The primary scientific goal is to provide a
comprehensive and uniform database of the main structural and photometric
parameters of the sample members from NIR surface photometry. To this end,
elliptical isophotal fitting was performed on each galaxy image to extract
information about the size and location of its morphological components and
provide the azimuthally averaged radial brightness profile. Analytical
functions for each component's brightness distribution were then used to match
that profile, and their functional parameters obtained from the global fitting.
This first report includes data for NGC 3344, NGC 3686, NGC 3938, NGC 3953, NGC
4254, NGC 4303, NGC 4314, NGC 5248, NGC 6384 and NGC 7479.
