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.
https://anaconda.org/r_test/r-sopie/badges/version.svg
https://anaconda.org/r_test/r-sopie/badges/latest_release_date.svg
https://anaconda.org/r_test/r-sopie/badges/latest_release_relative_date.svg
https://anaconda.org/r_test/r-sopie/badges/platforms.svg
https://anaconda.org/r_test/r-sopie/badges/license.svg
https://anaconda.org/r_test/r-sopie/badges/downloads.svg