Imprints of local lightcone projection effects on the galaxy bispectrum. Part II

General relativistic imprints on the galaxy bispectrum arise from observational (or projection) effects. The lightcone projection effects include local contributions from Doppler and gravitational potential terms, as well as lensing and other integrated contributions. We recently presented for the first time, the correction to the galaxy bispectrum from all local lightcone projection effects up to second order in perturbations. Here we provide the details underlying this correction, together with further results and illustrations. For moderately squeezed shapes, the correction to the Newtonian prediction is similar to 30% on equality scales at z similar to 1. We generalise our recent results to include the contribution, up to second order, of magni fi cation bias (which affects some of the local terms) and evolution bias.