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.
@article{arxiv.1803.09391,
title = {Have we seen all glitches?},
author = {Meng Yu},
journal= {arXiv preprint arXiv:1803.09391},
year = {2018}
}
Comments
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