TL;DR
This paper discusses the detection probability density of neutron star glitches in pulsar timing data, emphasizing its importance for understanding glitch detectability with specific observation setups.
Contribution
It extends previous work by further analyzing the detection probability density of glitches in pulsar data, providing deeper insights into glitch detectability.
Findings
Detection probability density is crucial for glitch detection.
Extended analysis of detection probability density in pulsar data.
Implications for optimizing pulsar observation schedules.
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.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements · Seismology and Earthquake Studies