The Kolmogorov-Smirnov Test is a non-parametric statistical method used to compare the distribution of a sample with a known distribution or with another sample.

Astrostatistics aims to extract meaningful insights from astronomical data, such as the distribution of stars, the evolution of galaxies, and the properties of celestial objects.

The Parallax Method is a trigonometric technique used to estimate the distance to a star by measuring its apparent shift in position as the Earth orbits the Sun.

The Log-Normal Distribution is a statistical model commonly used to describe the distribution of galaxies in the universe, as it can account for the observed skewed distribution.

Grubbs' Test, Chauvenet's Criterion, and Dixon's Q-Test are all statistical methods used to identify and remove outliers in astronomical data.

Bayesian inference is a statistical method that allows for the estimation of unknown parameters, making predictions about future observations, and testing hypotheses, all while incorporating prior knowledge and uncertainty.

ARIMA, Fourier Analysis, and Wavelet Analysis are all statistical techniques used to analyze the time series data of astronomical objects, such as the light curves of stars or the rotation periods of planets.

The p-value in astrostatistics represents the probability of obtaining a result as extreme or more extreme than the observed result, assuming the null hypothesis is true.

ANOVA is a statistical method used to compare the means of two or more groups, making it suitable for comparing the properties of astronomical populations.

Monte Carlo simulations are used in astrostatistics to generate synthetic data, estimate uncertainties, and test hypotheses, particularly when dealing with complex models or insufficient data.

Pearson Correlation Coefficient, Spearman's Rank Correlation Coefficient, and Kendall's Tau Correlation Coefficient are all statistical techniques used to identify correlations between astronomical variables.

Hierarchical Bayesian models are used in astrostatistics to incorporate prior knowledge and uncertainty, handle complex data structures, and improve computational efficiency.

Isochrone Fitting, Color-Magnitude Diagram Analysis, and Spectroscopic Analysis are all statistical methods used to estimate the age of a star cluster.

The AIC is a statistical measure that compares the goodness of fit of different models, penalizing models with more parameters to prevent overfitting.

Power Spectrum Analysis is a statistical technique used to analyze the distribution of matter in the universe by studying the fluctuations in the cosmic microwave background radiation.