  The simultaneous presence of variability due to both pulsations and binarity
is no rare phenomenon. Unfortunately, the complexities of dealing with even one
of these sources of variability individually means that the other signal is
often treated as a nuisance and discarded. However, both types of variability
offer means to probe fundamental stellar properties in robust ways through
asteroseismic and binary modelling. We present an efficient methodology that
includes both binary and asteroseismic information to estimate fundamental
stellar properties based on a grid-based modelling approach. We report
parameters for three gravity mode pulsating {\it Kepler} binaries , such as
mass, radius, age, as well the mass of the convective core and location of the
overshoot region. We discuss the presence of parameter degeneracies and the way
our methodology deals with them. We provide asteroseismically calibrated
isochrone-clouds to the community; these are a generalisation of isochrones
when allowing for different values of the core overshooting in the two
components of the binary.
