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Secondary {\gamma}-rays from intergalactic cascades may contribute toobservable spectra of blazars, also modifying observable angular and temporaldistributions. In this paper we briefly review basic features of intergalacticelectromagnetic cascade physics, suggest a new approximation for {\gamma}-raymean free path, consider angular patterns of magnetically broadened cascadeemission, and present an example of a fit to the observable blazar spectrum.

Intergalactic electromagnetic cascade component of observable blazar emission