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SOPIE (version 1.6)

Non-Parametric Estimation of the Off-Pulse Interval of a Pulsar

Description

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.

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Version

Install

install.packages('SOPIE')

Monthly Downloads

196

Version

1.6

License

GPL-3

Maintainer

Willem Schutte

Last Published

February 23rd, 2022

Functions in SOPIE (1.6)

crab

PSR J0534+2200 (Crab-Pulsar) Time of Arrivals
findh

Calculate the Estimated Smoothing Parameter
J1709

PSR J1709-44290 Time of Arrivals
SOPIE-package

Package 'SOPIE' : Summary Information
circ.kernel

Circular Kernel Density Estimation
a.estimate

Estimate the Left Endpoint of the Off-Pulse Interval of a Pulsar
simdata

Simulated Data from a Scaled Von Mises Distribution with Noise
SOPIE

Sequential Off-Pulse Interval Estimation of a Pulsar Light Curve
b.estimate

Estimate the Right Endpoint of the Off-Pulse Interval of a Pulsar
von_mises_sim

Generates Simulated Data from a Von Mises Distribution with Noise