Introduction.- Effective-one-body Hamiltonian in Scalar-Tensor Gravity at the Third postNewtonian order.- Nonlocal-in-time Effective-one-body Hamiltonian in Scalar-Tensor Theories at Third post-Newtonian order.- Gravitational Scattering up to Third post-Newtonian order for Conservative Dynamics in Scalar-Tensor Theories.- Angular Momentum Flux in Scalar-Tensor Theories up to 1.5 post-Newtonian order.- Radiation Reaction Force for Scalar-Tensor Theories in Effective-one-body Formalism.- Improving inference on neutron star properties using information from binary merger remnants.- Conclusions.
