  The galaxy bispectrum is affected on equality scales and above by
relativistic observational effects, at linear and nonlinear order. These
lightcone effects include local contributions from Doppler and gravitational
potential terms, as well as integrated contributions like lensing, together
with all the couplings at nonlinear order. We recently presented the correction
to the galaxy bispectrum from all local lightcone effects up to second order in
perturbations, using a plane-parallel approximation. Here we update our
previous result by including the effects from relativistic nonlinear dynamical
evolution. We show that these dynamical effects make a significant contribution
to the projection effects.
