Basic Analysis > Distributions > Statistical Details for the Distribution Platform > Statistical Details for Continuous Fit Distributions
Publication date: 07/08/2024

Statistical Details for Continuous Fit Distributions

This section contains statistical details for the options in the Continuous Fit menu in the Distribution platform. Unless otherwise specified, confidence intervals for parameter estimates use likelihood-based calculations. For more information about likelihood-based confidence intervals, see Statistical Details for Profile Likelihood Confidence Limits in Predictive and Specialized Modeling. If the Y column has a Detection Limits column property, the Continuous Fit options fit a censored distribution and only a subset of distributions are available. For more information about fitting distributions to censored data, see Meeker and Escobar (1998).

Fit Normal

The Fit Normal option estimates the two parameters of the normal distribution:

μ (the mean) defines the location of the distribution on the x-axis

σ (standard deviation) defines the dispersion or spread of the distribution

The standard normal distribution occurs when μ = 0 and σ = 1.

pdf: Equation shown here for Equation shown here; Equation shown here; 0 < σ

E(x) = μ

Var(x) = σ2

Note: Confidence intervals for the mean estimate are based on the t distribution. Confidence intervals for the scale parameter are based on the χ2 distribution.

Fit Cauchy

The Fit Cauchy option fits a Cauchy distribution with location μ and scale σ.

pdf: Equation shown here for Equation shown here; Equation shown here; 0 < σ

E(x) = undefined

Var(x) = undefined

Fit Student’s t

The Fit Student’s t option fits a Student’s t distribution with location μ, scale σ, and degrees of freedom ν.

pdf: Equation shown here for Equation shown here; Equation shown here; 0 < σ; 1 ≤ ν

E(x) = μ for 1 < ν

Var(x) = σ2ν/(ν-2) for 2 < ν

Note: When ν = 1, the Student’s t distribution is equivalent to the Cauchy distribution.

Fit SHASH

The Fit SHASH option fits a sinh-arcsinh (SHASH) distribution. The SHASH distribution is based on a transformation of the normal distribution and includes the normal distribution as a special case. It can be symmetric or asymmetric. The shape is determined by the two shape parameters, γ and δ. For more information about the SHASH distribution, see Jones and Pewsey (2009).

pdf: Equation shown here for Equation shown here; 0 < δ, σ

where

Equation shown here is the standard normal pdf

Equation shown here

When γ = 0 and δ = 1, the SHASH distribution is equivalent to the normal distribution with location θ and scale σ.

The transformation sinh(w) is normally distributed with μ = 0 and σ = 1.

Fit ZI SHASH

The Fit ZI SHASH option fits a zero-inflated (ZI) sinh-arcsinh (SHASH) distribution. The zero-inflated SHASH distribution is equivalent to a SHASH distribution with a point mass at zero. It can be symmetric or asymmetric.

pdf: Equation shown here for Equation shown here; 0 < δ, σ

where

Equation shown here is the standard normal pdf

Equation shown here

Note: Confidence intervals for ZI SHASH distribution parameter estimates use Wald-based calculations.

Fit Exponential

The exponential distribution is especially useful for describing events that randomly occur over time, such as survival data. The exponential distribution might also be useful for modeling elapsed time between the occurrence of non-overlapping events. Examples of non-overlapping events include the following: the time between a user’s computer query and response of the server, the arrival of customers at a service desk, or calls coming in at a switchboard.

The Exponential distribution is a special case of the two-parameter Weibull when β = 1 and α = σ, and also a special case of the Gamma distribution when α = 1.

pdf: Equation shown here for 0 < σ; 0 ≤ x

E(x) = σ

Var(x) = σ2

Devore (1995) notes that an exponential distribution is memoryless. Memoryless means that if you check a component after t hours and it is still working, the distribution of additional lifetime (the conditional probability of additional life given that the component has lived until t) is the same as the original distribution.

Fit ExGaussian

The Fit ExGaussian option fits a distribution that is the sum of a normal distribution and an exponential distribution. The ExGaussian option estimates the location, μ, and scale, σ, of the normal distribution portion and the exponential distribution parameter λ.

pdf: Equation shown here for Equation shown here; Equation shown here; 0 < σ, λ

where Φ(·) is the standard normal cdf.

E(x) = μ + 1/λ

Var(x) = σ2 + 1/λ2

For more information about the exponentially modified Gaussian distribution, see Ament et al. (2019) and Palmer et al. (2011). Note that the parameterization of the exponential portion of the distribution differs in some sources. The parameterization in the Fit ExGaussian option uses the reciprocal of the parameterization that is used in the Fit Exponential option in the Distribution platform.

Fit Gamma

The Fit Gamma option estimates the gamma distribution parameters, α > 0 and σ > 0. The parameter α, called alpha in the fitted gamma report, describes shape or curvature. The parameter σ, called sigma, is the scale parameter of the distribution. The data must be greater than zero.

pdf: Equation shown here for 0 < x; 0 < α, σ

E(x) = ασ

Var(x) = ασ2

The standard gamma distribution has σ = 1. Sigma is called the scale parameter because values other than 1 stretch or compress the distribution along the horizontal axis.

The chi-square Equation shown here distribution occurs when σ = 2 and α = ν/2.

The exponential distribution occurs when α = 1.

The standard gamma density function is strictly decreasing when α ≤ 1. When α > 1, the density function begins at zero, increases to a maximum, and then decreases.

Fit Lognormal

The Fit Lognormal option estimates the parameters μ (scale) and σ (shape) for the two-parameter lognormal distribution. A variable Y is lognormal if and only if X = ln(Y) is normal. The data must be greater than zero.

pdf: Equation shown here for Equation shown here; Equation shown here; 0 < σ

E(x) = Equation shown here

Var(x) = Equation shown here

Fit Weibull

The Weibull distribution has different shapes depending on the values of α (scale) and β (shape). It often provides a good model for estimating the length of life, especially for mechanical devices and in biology.

The pdf for the Weibull distribution is defined as follows:

pdf: Equation shown here for α,β > 0; 0 < x

E(x) = Equation shown here

Var(x) = Equation shown here

where Γ(·) is the Gamma function.

Fit Normal 2 Mixture and Fit Normal 3 Mixture

The Fit Normal 2 Mixture and Fit Normal 3 Mixture options fit a mixture of two or three normal distributions. These flexible distributions are capable of fitting bimodal or multi-modal data. A separate mean, standard deviation, and proportion of the whole is estimated for each group. In the following equations, k equals the number of normal distributions in the mixture.

pdf: Equation shown here

E(x) =Equation shown here

Var(x) =Equation shown here

where μi, σi, and πi are the respective mean, standard deviation, and proportion for the ith group, and φ(·) is the standard normal pdf.

Note: Confidence intervals for normal mixture distribution parameter estimates use Wald-based calculations.

Fit Johnson

The Fit Johnson option selects and fits the best-fitting distribution from the Johnson system of distributions, which contains three distributions that are all based on a transformed normal distribution. These three distributions are the following:

Johnson Su, which is unbounded.

Johnson Sb, which has bounds on both tails. The bounds are defined by parameters that can be estimated.

Johnson Sl, which is bounded in one tail. The bound is defined by a parameter that can be estimated. The Johnson Sl family contains the family of lognormal distributions.

Only the fit for the selected distribution is reported. Information about selection procedures and parameter estimation for the Johnson distributions can be found in Slifker and Shapiro (1980). The parameter estimation does not use maximum likelihood.

Johnson distributions are popular because of their flexibility. In particular, the Johnson distribution system is noted for its data-fitting capabilities because it supports every possible combination of skewness and kurtosis. However, the SHASH distribution is also very flexible and is recommended over the Johnson distributions.

If Z is a standard normal variate, then the system is defined as follows:

Equation shown here

where, for the Johnson Su:

Equation shown here

Equation shown here

where, for the Johnson Sb:

Equation shown here

Equation shown here

and for the Johnson Sl, where σ = ±1.

Equation shown here

Equation shown here

Johnson Su

pdf: Equation shown here for - < x, θ, γ < ; 0 < θ,δ

Johnson Sb

pdf: Equation shown here for θ < x < θ+σ; 0 < σ

Johnson Sl

pdf: Equation shown here for θ < x if σ = 1; θ > x if σ = -1

where φ(·)is the standard normal pdf.

Note: Confidence intervals for Johnson distribution parameter estimates use Wald-based calculations.

Fit Beta

The beta distribution is useful for modeling the behavior of random variables that are constrained to fall in the interval 0,1. For example, proportions always fall between 0 and 1. The Fit Beta option estimates two shape parameters, α > 0 and β > 0. The beta distribution has values only in the interval 0,1.

pdf: Equation shown here for 0 < x < 1; 0 < σ,α,β

E(x) = Equation shown here

Var(x) = Equation shown here

where B(·) is the Beta function.

Fit All

In the Compare Distributions report, the Distribution list is sorted by AICc in ascending order. Use the check boxes to show or hide a fit report and overlay curve for the selected distribution.

The formulas for AICc and BIC are defined as follows:

AICc = Equation shown here

BIC = Equation shown here

where:

logL is the log-likelihood.

n is the sample size.

k is the number of parameters.

The AICc Weight column shows normalized AICc values that sum to one. The AICc weight can be interpreted as the probability that a particular distribution is the true distribution given that one of the fitted distributions is the truth. Therefore, the distribution with the AICc weight closest to one is the better fit. The AICc weights are calculated using only nonmissing AICc values:

AICcWeight = exp[-0.5(AICc-min(AICc))] / sum(exp[-0.5(AICc-min(AICc))])

where min(AICc) is the smallest AICc value among the fitted distributions.

For more information about the measures in the Compare Distributions report, see Likelihood, AICc, and BIC in Fitting Linear Models.

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