  The GHASP survey (Gassendi HAlpha survey of SPirals) consists of 3D Ha data
cubes for 203 spiral and irregular galaxies, covering a large range in
morphological types and absolute magnitudes, for kinematics analysis. It is the
largest sample of Fabry-Perot data published up to now. In order to provide an
homogenous sample, reduced and analyzed using the same procedure, we present in
this paper the new reduction and analysis for a set of 97 galaxies already
published in previous papers but now using the new data reduction procedure
adopted for the whole sample. The GHASP survey is now achieved and the whole
sample is reduced using adaptive binning techniques based on Voronoi
tessellations. We have derived Ha data cubes from which are computed Ha maps,
radial velocity fields as well as residual velocity fields, position-velocity
diagrams, rotation curves and kinematical parameters for almost all galaxies.
The rotation curves, the kinematical parameters and their uncertainties are
computed homogeneously using the new method based on the power spectrum of the
residual velocity field. This paper provides the kinematical parameters for the
whole sample. For the first time, the integrated Ha profiles have been computed
and are presented for the whole sample. The total Ha fluxes deduced from these
profiles have been used in order to provide a flux calibration for the 203
GHASP galaxies. This paper confirms the conclusions already drawn from half the
sample concerning (i) the increased accuracy of position angles measurements
using kinematical data, (ii) the difficulty to have robust determinations of
both morphological and kinematical inclinations in particular for low
inclination galaxies and (iii) the very good agreement between the Tully-Fisher
relationship derived from our data and previous determinations.
