# Have we seen all glitches?

## 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.

## Key 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.