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Provides functions to non-parametrically estimate the off-pulse interval of a source function originating from a pulsar. The technique is based on a sequential application of P-values obtained from goodness-of-fit tests for the uniform distribution, such as the Kolmogorov-Smirnov, Cramer-von Mises, Anderson-Darling and Rayleigh goodness-of-fit tests.
Package details |
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Author | Willem Daniel Schutte |
Maintainer | Willem Daniel Schutte <wd.schutte@nwu.ac.za> |
License | GPL-3 |
Version | 1.6 |
Package repository | View on CRAN |
Installation |
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