Have we seen all glitches?

Abstract

Neutron star glitches are observed via artificially scheduled pulsar pulse arrival-time observations. Detection probability density of glitch events for a given data set is essentially required knowledge for realizing glitch detectability with specified observing system and schedule. In Yu & Liu, the detection probability density was derived for the Yu et al. data set. In this proceeding, further discussions are presented.

Has appeared in the conference proceeding of 'Stars with magnetic field: from pre-main sequence to compact remnants', Aug. 28 - Sept. 1, 2017, Brno, Czech