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The galaxy bispectrum on scales around and above the equality scale receivescontributions from relativistic effects. Some of these arise from lightconedeformation effects, which come from local and line-of-sight integratedcontributions. Here we calculate the local contributions from the generatedvector and tensor background which is formed as scalar modes couple and enterthe horizon. We show that these modes are sub-dominant when compared with otherrelativistic contributions.

Imprints of local lightcone projection effects on the galaxy bispectrum IV: Second-order vector and tensor contributions