  We present the list of variable stars we found in the \kep\ superstamp data
covering approximately nine arcminutes from the central region of NGC6819. This
is a continuation of our work presented by Sanjayan et al.(2022a). We
classified the variable stars based on the variability type and we established
their cluster membership based on the available Gaia Data Release 3 astrometry.
Our search revealed 385 variable stars but only 128 were found to be cluster
members. In the case of eclipsing and contact binaries we calculated the
mid-times of eclipses and derived ephemerides. We searched for eclipse timing
variation using the observed minus calculated diagrams. Only five objects show
significant orbital period variation. We used isochrones calculated within the
MESA Isochrones and Stellar Tracks project and derived the average age (2.54
Gyr), average distance (2.3 kpc) and iron content [Fe/H] = -0.01(2), of
NGC6819. We confirm this distance by the one derived from Gaia astrometry of
the cluster members with membership probabilities greater than 0.9.
