My assumed definition of angular momentum is the sum over $i$ of $L_i =r_i\times{\omega_i}\times{r_i}$ for each particle about some origin.
We have two spheres rotating about the centre of orbit. For simplicity's sake, let's assume it is the centre of the earth. The moon has an orbit rate of $\omega_{m1}$ and a spin rate of $\omega_{m2}$. It is spinning around its own axis which passes through the centre of the moon, this axis is parallel to the axis it orbits about. The earth spins about an axis that is tilted at some angle to the axis of the moon's orbit.
what is the angular momentum of the moon, in terms of its mass, radius, distance to earth's centre, and its angular velocities?
This question answers my conceptual query of how rotation about a parallel axis affects angular momentum. I have derived the relation for when the rotation acts about an axis passing through the origin. $L_i = \omega r_i\cdot{r_i}-r_i\omega\cdot{r_i}$ which is obviously $I\omega$ since $\omega$ is constant. This tells us that the A.M of the earth is simply given by the formula of the momentum of inertia of a sphere times its angular velocity, given the initial assumption. However, it is not trivial to say that this stays the same when the system is shifted to the right for the moon.