Non-Parametric Estimation of the Off-Pulse Interval of a Pulsar
Estimate the Left Endpoint of the Off-Pulse Interval of a Pulsar
Estimate the Right Endpoint of the Off-Pulse Interval of a Pulsar
Circular Kernel Density Estimation
Calculate the Estimated Smoothing Parameter
Package 'SOPIE' : Summary Information
Sequential Off-Pulse Interval Estimation of a Pulsar Light Curve
Generates Simulated Data from a Von Mises Distribution with Noise
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.