2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/5261We present high-time-resolution observations of the young precessing pulsar B1828-11, which yield clues to the true beam shape and the fundamental precession period.4 pages; to appear in proceedings of "Radio Pulsars," eds. M. Bailes, D. J. Nice, S. E. ThorsettAstrophysicstext