CAOSP abstracts, Volume: 48, No.: 1, year: 2018

Abstract: Neutron star glitches are observed via artificially scheduled pulsar pulse arrival-time observations. The detection probability density of glitch events for a given data set is an essentially required knowledge for realizing glitch detectability with a specified observing system and schedule. In Yu & Liu (2017), the detection probability density was derived for the Yu et al. (2013) data set. In this proceeding, further discussions are presented.

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Last update: February 06, 2018