Timing solutions for five PALFA rotating radio transients, spin periods for two more, and Bayesian energy and wait-time fits that support log-normal burst energies and near-Poisson burst times.
Problems with Fitting to the Power-Law Distribution
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
This short communication uses a simple experiment to show that fitting to a power law distribution by using graphical methods based on linear fit on the log-log scale is biased and inaccurate. It shows that using maximum likelihood estimation (MLE) is far more robust. Finally, it presents a new table for performing the Kolmogorov-Smirnof test for goodness-of-fit tailored to power-law distributions in which the power-law exponent is estimated using MLE. The techniques presented here will advance the application of complex network theory by allowing reliable estimation of power-law models from data and further allowing quantitative assessment of goodness-of-fit of proposed power-law models to empirical data.
fields
astro-ph.HE 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Timing and statistical analysis of single-pulse search pulsar discoveries from the PALFA survey
Timing solutions for five PALFA rotating radio transients, spin periods for two more, and Bayesian energy and wait-time fits that support log-normal burst energies and near-Poisson burst times.