Simulation and Estimation Diagnostics

Model diagnostics are used to check if the model fits the data well. Diagnostics for continuous data are different from for discrete data.

The inspect Function

The main function to call when looking at diagnostics from a fit is inspect with the signature:

Pumas.inspect — Function
inspect(fpm::AbstractFittedPumasModel; wres_approx::LikelihoodApproximation, nsim::Int, rng)

Output a summary of the model predictions, residuals, Empirical Bayes estimates, and NPDEs (when requested).

Called on a fit output and allows the keyword argument wres_approx for approximation method to be used in residual calculation. The default value is the approximation method used for the marginal likelihood calculation in the fit that produced fpm. The keyword nsim controls the number of times each subject is simulated for npde computation. A FittedPumasModelInspection object with pred, wres, ebes, and npdes is output.

The function outputs a summary of the model predictions, residuals, Empirical Bayes estimates, and NPDEs (when requested). It is called on a fit output and allows the keyword argument wres_approx for approximation method to be used in residual calculation. The default value is the approximation method used for the marginal likelihood calculation in the fit that produced fpm. The keyword nsim controls the number of times each subject is simulated for the npde computations. rng is a random number generator that can be used to seed any random elements such as those in npde computations.

inspect returns a FittedPumasModelInspection object with the

  • model predictions
  • residuals
  • empirical Bayes estimates
  • individual coefficients
  • dose control parameters

Example syntax

my_inspect = DataFrame(inspect(my_fit))

The result of inspect(my_fit) is a FittedPumasModelInspection object, which can then be converted into tabular form using the DataFrame call. This is useful if one is interested to export the results into a spreadsheet, or use the resulting DataFrame for plotting.

Weighted Residuals

In Pumas, you can calculate individual and population weighted residuals using wresiduals as well as expected individual weighted residuals with the signature

Pumas.wresiduals — Function
wresiduals(fpm::AbstractFittedPumasModel, approx::LikelihoodApproximation; nsim=nothing)

Calculate the individual and population weighted residual.

Takes a fit result, an approximation method for the marginal likelihood calculation which defaults to the method used in the fit and the number of simulations with the keyword argument nsim. If nsim is specified only the Expected Simulation based Individual Weighted Residuals (EIWRES) is included in the output as individual residual and population residual is not computed. Using the FO approximation method corresponds to the WRES and while FOCE(I) corresponds to CWRES. The output is a SubjectResidual object that stores the population (wres) and individual (iwres) residuals along with the subject and approximation method (approx).

Takes a fit result, an approximation method for the marginal likelihood calculation which defaults to the method used in the fit and the number of simulations with the keyword argument nsim. If nsim is specified only the Expected Simulation based Individual Weighted Residuals (EIWRES) is included in the output as individual residual and population residual is not computed. Using the FO approximation method corresponds to the WRES and while FOCE corresponds to CWRES. The output is a SubjectResidual object that stores the population (wres) and individual (iwres) residuals along with the subject and approximation method (approx).

Predictions

To calculate predictions from a fit use the predict function with the signature:

StatsAPI.predict — Function
predict(
  model::AbstractPumasModel,
  subject::Subject,
  param::NamedTuple,
  [randeffs,];
  [obstimes::AbstractVector,
  diffeq_options::NamedTuple]
)::Union{SubjectPrediction,Vector{SubjectPrediction}}

Compute population and individual predictions for the single subject based on model and the population parameters param. A NamedTuple of random effects, randeffs, can be omitted or provided by the user. If they are omitted, they will be estimated from the data in the subject.

If the optional obstimes argument is passed then the time points in obstimes are used for the predictions. Otherwise, the time points of the observations of the subject are used for the predictions.

The function allows for extra keyword arguments to be passed on to the differential equations solver through the diffeq_options keyword. See the online documentation for more details.

predict(
  fpm::AbstractFittedPumasModel,
  [population::Union{Subject,Population}];
  [obstimes::AbstractVector]
)::Union{SubjectPrediction,Vector{SubjectPrediction}}

Compute population and individual predictions for the fitted model fpm. By default, the predictions are computed for the estimation data but the predictions can also be computed for user supplied data by passing either a single subject or a vector of subjects (Population) as the population argument.

If the optional obstimes argument is passed then the time points in obstimes are used for the predictions. Otherwise, the time points of the observations for each subject in the population are used for the predictions.

Any optional keyword arguments used when fitting fpm are reused when computing the predictions.

By default, the predictions are computed for the estimation data, but the predictions can also be computed for user supplied data by passing either a single subject or a vector of subjects (Population) as the population argument. If the optional obstimes argument is passed then the time points in obstimes are used for the predictions. Otherwise, the time points of the observations for each subject in the population are used for the predictions.

Any optional keyword arguments used when fitting fpm are reused when computing the predictions.

Model Metrics

Akaike information criterion:

StatsAPI.aic — Function
aic(fpm::AbstractFittedPumasModel)

Calculate the Akaike information criterion (AIC) of the fitted Pumas model fpm.

Bayesian information criterion:

StatsAPI.bic — Function
bic(fpm::AbstractFittedPumasModel)

Calculate the Bayesian information criterion (BIC) of the fitted Pumas model fpm.

Shrinkage

Pumas.ηshrinkage — Function
ηshrinkage(fpm::AbstractFittedPumasModel)

Calculate the η-shrinkage.

Takes the result of a fit as the only input argument. A named tuple of the random effects and corresponding η-shrinkage values is output.

Pumas.ϵshrinkage — Function
ϵshrinkage(fpm::AbstractFittedPumasModel)

Calculate the ϵ-shrinkage.

Takes the result of a fit as the only input argument. A named tuple of derived variables and corresponding ϵ-shrinkage values is output.

If the observations for an individual is informative, η-shrinkage will be low. If, on the other hand, the observations are non-informative, the individual estimates (EBEs) will shrink towards the population mean. Hence, the variance of the EBEs will also shrink and η-shrinkage will be high.

When data gets sparse the IWRES distribution also shrink towards it’s mean (zero). This is often called overfitting or ϵ-shrinkage.