Statistical Estimates of the Pulsar Glitch Activity
A common way to calculate the glitch activity of a pulsar is an ordinary linear regression of the observed cumulative glitch history. This method however is likely to underestimate the errors on the activity, as it implicitly assumes a (long-term) linear dependence between glitch sizes and waiting t...
Main Authors: | , , , |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2021-01-01
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Series: | Universe |
Subjects: | |
Online Access: | https://www.mdpi.com/2218-1997/7/1/8 |