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.
|Author||Willem Daniel Schutte|
|Maintainer||Willem Daniel Schutte <[email protected]>|
|Package repository||View on CRAN|
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