vi_model: Model-specific variable importance

In vip: Variable Importance Plots

Model-specific variable importance

Description

Compute model-specific variable importance scores for the predictors in a fitted model.

Usage

vi_model(object, ...)

## Default S3 method:
vi_model(object, ...)

## S3 method for class 'C5.0'
vi_model(object, type = c("usage", "splits"), ...)

## S3 method for class 'train'
vi_model(object, ...)

## S3 method for class 'cubist'
vi_model(object, ...)

## S3 method for class 'earth'
vi_model(object, type = c("nsubsets", "rss", "gcv"), ...)

## S3 method for class 'gbm'
vi_model(object, type = c("relative.influence", "permutation"), ...)

## S3 method for class 'glmnet'
vi_model(object, lambda = NULL, ...)

## S3 method for class 'cv.glmnet'
vi_model(object, lambda = NULL, ...)

## S3 method for class 'H2OBinomialModel'
vi_model(object, ...)

## S3 method for class 'H2OMultinomialModel'
vi_model(object, ...)

## S3 method for class 'H2ORegressionModel'
vi_model(object, ...)

## S3 method for class 'lgb.Booster'
vi_model(object, type = c("gain", "cover", "frequency"), ...)

## S3 method for class 'mixo_pls'
vi_model(object, ncomp = NULL, ...)

## S3 method for class 'mixo_spls'
vi_model(object, ncomp = NULL, ...)

## S3 method for class 'WrappedModel'
vi_model(object, ...)

## S3 method for class 'Learner'
vi_model(object, ...)

## S3 method for class 'nn'
vi_model(object, type = c("olden", "garson"), ...)

## S3 method for class 'nnet'
vi_model(object, type = c("olden", "garson"), ...)

## S3 method for class 'RandomForest'
vi_model(object, type = c("accuracy", "auc"), ...)

## S3 method for class 'constparty'
vi_model(object, ...)

## S3 method for class 'cforest'
vi_model(object, ...)

## S3 method for class 'mvr'
vi_model(object, ...)

## S3 method for class 'mixo_pls'
vi_model(object, ncomp = NULL, ...)

## S3 method for class 'mixo_spls'
vi_model(object, ncomp = NULL, ...)

## S3 method for class 'WrappedModel'
vi_model(object, ...)

## S3 method for class 'Learner'
vi_model(object, ...)

## S3 method for class 'randomForest'
vi_model(object, ...)

## S3 method for class 'ranger'
vi_model(object, ...)

## S3 method for class 'rpart'
vi_model(object, ...)

## S3 method for class 'mlp'
vi_model(object, type = c("olden", "garson"), ...)

## S3 method for class 'ml_model_decision_tree_regression'
vi_model(object, ...)

## S3 method for class 'ml_model_decision_tree_classification'
vi_model(object, ...)

## S3 method for class 'ml_model_gbt_regression'
vi_model(object, ...)

## S3 method for class 'ml_model_gbt_classification'
vi_model(object, ...)

## S3 method for class 'ml_model_generalized_linear_regression'
vi_model(object, ...)

## S3 method for class 'ml_model_linear_regression'
vi_model(object, ...)

## S3 method for class 'ml_model_random_forest_regression'
vi_model(object, ...)

## S3 method for class 'ml_model_random_forest_classification'
vi_model(object, ...)

## S3 method for class 'lm'
vi_model(object, type = c("stat", "raw"), ...)

## S3 method for class 'model_fit'
vi_model(object, ...)

## S3 method for class 'workflow'
vi_model(object, ...)

## S3 method for class 'xgb.Booster'
vi_model(object, type = c("gain", "cover", "frequency"), ...)

Arguments

object	A fitted model object (e.g., a randomForest object). See the details section below to see how variable importance is computed for supported model types.
...	Additional optional arguments to be passed on to other methods. See the details section below for arguments that can be passed to specific object types.
type	Character string specifying the type of variable importance to return (only used for some models). See the details section below for which methods this argument applies to.
lambda	Numeric value for the penalty parameter of a glmnet model (this is equivalent to the s argument in coef.glmnet). See the section on glmnet in the details below.
ncomp	An integer for the number of partial least squares components to be used in the importance calculations. If more components are requested than were used in the model, all of the model's components are used.

Details

Computes model-specific variable importance scores depending on the class of object:

• C5.0 - Variable importance is measured by determining the percentage of training set samples that fall into all the terminal nodes after the split. For example, the predictor in the first split automatically has an importance measurement of 100 percent since all samples are affected by this split. Other predictors may be used frequently in splits, but if the terminal nodes cover only a handful of training set samples, the importance scores may be close to zero. The same strategy is applied to rule-based models and boosted versions of the model. The underlying function can also return the number of times each predictor was involved in a split by using the option metric = "usage". See C5imp for details.

• cubist - The Cubist output contains variable usage statistics. It gives the percentage of times where each variable was used in a condition and/or a linear model. Note that this output will probably be inconsistent with the rules shown in the output from summary.cubist. At each split of the tree, Cubist saves a linear model (after feature selection) that is allowed to have terms for each variable used in the current split or any split above it. Quinlan (1992) discusses a smoothing algorithm where each model prediction is a linear combination of the parent and child model along the tree. As such, the final prediction is a function of all the linear models from the initial node to the terminal node. The percentages shown in the Cubist output reflects all the models involved in prediction (as opposed to the terminal models shown in the output). The variable importance used here is a linear combination of the usage in the rule conditions and the model. See summary.cubist and varImp for details.

• glmnet - Similar to (generalized) linear models, the absolute value of the coefficients are returned for a specific model. It is important that the features (and hence, the estimated coefficients) be standardized prior to fitting the model. You can specify which coefficients to return by passing the specific value of the penalty parameter via the lambda argument (this is equivalent to the s argument in coef.glmnet). By default, lambda = NULL and the coefficients corresponding to the final penalty value in the sequence are returned; in other words, you should ALWAYS SPECIFY lambda! For cv.glmnet objects, the largest value of lambda such that the error is within one standard error of the minimum is used by default. For a multinomial response, the coefficients corresponding to the first class are used; that is, the first component of coef.glmnet.

• cforest - Variable importance is measured in a way similar to those computed by importance. Besides the standard version, a conditional version is available that adjusts for correlations between predictor variables. If conditional = TRUE, the importance of each variable is computed by permuting within a grid defined by the predictors that are associated (with 1 - p-value greater than threshold) to the variable of interest. The resulting variable importance score is conditional in the sense of beta coefficients in regression models, but represents the effect of a variable in both main effects and interactions. See Strobl et al. (2008) for details. Note, however, that all random forest results are subject to random variation. Thus, before interpreting the importance ranking, check whether the same ranking is achieved with a different random seed - or otherwise increase the number of trees ntree in ctree_control. Note that in the presence of missings in the predictor variables the procedure described in Hapfelmeier et al. (2012) is performed. See varimp for details.

• earth - The earth package uses three criteria for estimating the variable importance in a MARS model (see evimp for details):

  • The nsubsets criterion (type = "nsubsets") counts the number of model subsets that include each feature. Variables that are included in more subsets are considered more important. This is the criterion used by summary.earth to print variable importance. By "subsets" we mean the subsets of terms generated by earth()'s backward pass. There is one subset for each model size (from one to the size of the selected model) and the subset is the best set of terms for that model size. (These subsets are specified in the ⁠$prune.terms⁠ component of earth()'s return value.) Only subsets that are smaller than or equal in size to the final model are used for estimating variable importance. This is the default method used by vi_model.

  • The rss criterion (type = "rss") first calculates the decrease in the RSS for each subset relative to the previous subset during earth()’s backward pass. (For multiple response models, RSS's are calculated over all responses.) Then for each variable it sums these decreases over all subsets that include the variable. Finally, for ease of interpretation the summed decreases are scaled so the largest summed decrease is 100. Variables which cause larger net decreases in the RSS are considered more important.

  • The gcv criterion (type = "gcv") is similar to the rss approach, but uses the GCV statistic instead of the RSS. Note that adding a variable can sometimes increase the GCV. (Adding the variable has a deleterious effect on the model, as measured in terms of its estimated predictive power on unseen data.) If that happens often enough, the variable can have a negative total importance, and thus appear less important than unused variables.

• gbm - Variable importance is computed using one of two approaches (See summary.gbm for details):

  • The standard approach (type = "relative.influence") described in Friedman (2001). When distribution = "gaussian" this returns the reduction of squared error attributable to each variable. For other loss functions this returns the reduction attributable to each variable in sum of squared error in predicting the gradient on each iteration. It describes the relative influence of each variable in reducing the loss function. This is the default method used by vi_model.

  • An experimental permutation-based approach (type = "permutation"). This method randomly permutes each predictor variable at a time and computes the associated reduction in predictive performance. This is similar to the variable importance measures Leo Breiman uses for random forests, but gbm currently computes using the entire training dataset (not the out-of-bag observations).

• H2OModel - See h2o.varimp or visit https://docs.h2o.ai/h2o/latest-stable/h2o-docs/variable-importance.html for details.

• nnet - Two popular methods for constructing variable importance scores with neural networks are the Garson algorithm (Garson 1991), later modified by Goh (1995), and the Olden algorithm (Olden et al. 2004). For both algorithms, the basis of these importance scores is the network’s connection weights. The Garson algorithm determines variable importance by identifying all weighted connections between the nodes of interest. Olden’s algorithm, on the other hand, uses the product of the raw connection weights between each input and output neuron and sums the product across all hidden neurons. This has been shown to outperform the Garson method in various simulations. For DNNs, a similar method due to Gedeon (1997) considers the weights connecting the input features to the first two hidden layers (for simplicity and speed); but this method can be slow for large networks.. To implement the Olden and Garson algorithms, use type = "olden" and type = "garson", respectively. See garson and olden for details.

• lm/glm - In (generalized) linear models, variable importance is typically based on the absolute value of the corresponding t-statistics (Bring, 1994). For such models, the sign of the original coefficient is also returned. By default, type = "stat" is used; however, if the inputs have been appropriately standardized then the raw coefficients can be used with type = "raw". Note that Bring (1994) provides motivation for using the absolute value of the associated t-statistics.

• sparklyr - The Spark ML library provides standard variable importance measures for tree-based methods (e.g., random forests). See ml_feature_importances for details.

• randomForest Random forests typically provide two measures of variable importance.

  • The first measure is computed from permuting out-of-bag (OOB) data: for each tree, the prediction error on the OOB portion of the data is recorded (error rate for classification and MSE for regression). Then the same is done after permuting each predictor variable. The difference between the two are then averaged over all trees in the forest, and normalized by the standard deviation of the differences. If the standard deviation of the differences is equal to 0 for a variable, the division is not done (but the average is almost always equal to 0 in that case).

  • The second measure is the total decrease in node impurities from splitting on the variable, averaged over all trees. For classification, the node impurity is measured by the Gini index. For regression, it is measured by residual sum of squares.

  See importance for details, including additional arguments that can be passed via the ... argument in vi_model.

• cforest - Same approach described in cforest (from package partykit) above. See varimp and varimpAUC (if type = "auc") for details.

• ranger - Variable importance for ranger objects is computed in the usual way for random forests. The approach used depends on the importance argument provided in the initial call to ranger. See importance for details.

• rpart - As stated in one of the rpart vignettes. A variable may appear in the tree many times, either as a primary or a surrogate variable. An overall measure of variable importance is the sum of the goodness of split measures for each split for which it was the primary variable, plus "goodness" * (adjusted agreement) for all splits in which it was a surrogate. Imagine two variables which were essentially duplicates of each other; if we did not count surrogates, they would split the importance with neither showing up as strongly as it should. See rpart for details.

• caret - Various model-specific and model-agnostic approaches that depend on the learning algorithm employed in the original call to caret. See varImp for details.

• xgboost - For linear models, the variable importance is the absolute magnitude of the estimated coefficients. For that reason, in order to obtain a meaningful ranking by importance for a linear model, the features need to be on the same scale (which you also would want to do when using either L1 or L2 regularization). Otherwise, the approach described in Friedman (2001) for gbms is used. See xgb.importance for details. For tree models, you can obtain three different types of variable importance:

  • Using type = "gain" (the default) gives the fractional contribution of each feature to the model based on the total gain of the corresponding feature's splits.

  • Using type = "cover" gives the number of observations related to each feature.

  • Using type = "frequency" gives the percentages representing the relative number of times each feature has been used throughout each tree in the ensemble.

• lightgbm - Same as for xgboost models, except lgb.importance (which this method calls internally) has an additional argument, percentage, that defaults to TRUE, resulting in the VI scores shown as a relative percentage; pass percentage = FALSE in the call to vi_model() to produce VI scores for lightgbm models on the raw scale.

Value

A tidy data frame (i.e., a tibble object) with two columns:

• Variable - the corresponding feature name;

• Importance - the associated importance, computed as the average change in performance after a random permutation (or permutations, if nsim > 1) of the feature in question.

For lm/glm-like objects, the sign (i.e., POS/NEG) of the original coefficient is also included in a column called Sign.

Note

Inspired by the caret's varImp function.

Source

Johan Bring (1994) How to Standardize Regression Coefficients, The American Statistician, 48:3, 209-213, DOI: 10.1080/00031305.1994.10476059.

Examples

## Not run: 
# Basic example using imputed titanic data set
t3 <- titanic_mice[[1L]]

# Fit a simple model
set.seed(1449)  # for reproducibility
bst <- lightgbm::lightgbm(
  data = data.matrix(subset(t3, select = -survived)),
  label = ifelse(t3$survived == "yes", 1, 0),
  params = list("objective" = "binary", "force_row_wise" = TRUE),
  verbose = 0
)

# Compute VI scores
vi(bst)  # defaults to `method = "model"`
vi_model(bst)  # same as above

# Same as above (since default is `method = "model"`), but returns a plot
vip(bst, geom = "point")
vi_model(bst, type = "cover")
vi_model(bst, type = "cover", percentage = FALSE)

# Compare to
lightgbm::lgb.importance(bst)

## End(Not run)

vip documentation built on Aug. 21, 2023, 5:12 p.m.