Generalized Linear Model (GLM)¶
Introduction¶
Generalized Linear Models (GLM) estimate regression models for outcomes following exponential distributions. In addition to the Gaussian (i.e. normal) distribution, these include Poisson, binomial, and gamma distributions. Each serves a different purpose, and depending on distribution and link function choice, can be used either for prediction or classification.
The GLM suite includes:
Gaussian regression
Poisson regression
Binomial regression (classification)
Fractional binomial regression
Quasibinomial regression
Multinomial classification
Gamma regression
Ordinal regression
Negative Binomial regression
Tweedie distribution
Additional Resources¶
Defining a GLM Model¶
Parameters are optional unless specified as required.
Algorithmspecific parameters¶
build_null_model: If set, will build a model with only the intercept. This option defaults to
False
.calc_like: Specify whether to return likelihood function value for HGLM or normal GLM. Setting this option to
True
while disablingHGLM
will enable the calculation of the full log likelihood and full AIC. This option defaults toFalse
(disabled).custom_metric_func: Specify a custom evaluation function.
dispersion_epsilon: If changes in dispersion parameter estimation or loglikelihood value is smaller than
dispersion_epsilon
, this will break out of the dispersion parameter estimation loop using maximum likelihood. This option defaults to0.0001
.dispersion_learning_rate: (Applicable only when
dispersion_parameter_method="ml"
) This value controls how much the dispersion parameter estimate will be changed when the calculated loglikelihood actually decreases with the new dispersion. In this case, instead of setting dispersion = dispersion + change, it is dispersion + dispersion_learning_rate \(\times\) change. This option must be > 0 and defaults to0.5
.dispersion_parameter_method: Method used to estimate the dispersion factor for Tweedie, Gamma, and Negative Binomial only. Can be one of
"pearson"
(default),"deviance"
, or"ml"
.fix_dispersion_parameter: Only used for Tweedie, Gamma and Negative Binomial GLM. If enabled, this option will use the dispsersion parameter in
init_dispersion_parameter
as the standard error and use it to calculate the pvalues. This option defaults toFalse
.generate_scoring_history: Generate the scoring history for the GLM model when enabled. This may significantly slow down the algorithm. When enabled, you will also be able to fetch the average objective and the negative log likelihood using their accessor functions:
average_objective
andnegative_log_likelihood
. This option defaults toFalse
(disabled).generate_variable_inflation_factors: If enabled, this option generates the variable inflation factors for numerical predictors. This option defaults to
False
(disabled).init_dispersion_parameter: Initial value of disperion factor before being estimated using either
"pearson"
or"ml"
. This option defaults to1.0
.interactions: Specify a list of predictor column indices to interact. All pairwise combinations will be computed for this list.
interaction_pairs: When defining interactions, use this option to specify a list of pairwise column interactions (interactions between two variables). Note that this is different than
interactions
, which will compute all pairwise combinations of specified columns.max_iterations_dispersion: Control the maximum number of iterations in the dispersion parameter estimation loop using maximum likelihood. This option defaults to
1000000
.rand_family: The Random Component Family specified as an array. You must include one family for each random component. Currently only
rand_family=["gaussisan"]
is supported.upload_custom_metric: Upload a custom metric into a running H2O cluster.
HGLM parameters¶
HGLM: If enabled, then an HGLM model will be built. If disabled (default), then a GLM model will be built.
rand_link: The link function for random component in HGLM specified as an array. Available options include
identity
andfamily_default
.random_columns: An array of random column indices to be used for
HGLM
.startval: The initial starting values for fixed and randomized coefficients in
HGLM
specified as a double array.
Common parameters¶
auc_type: Set the default multinomial AUC type. Must be one of:
"AUTO"
(default)"NONE"
"MACRO_OVR"
"WEIGHTED_OVR"
"MACRO_OVO"
"WEIGHTED_OVO"
checkpoint: Enter a model key associated with a previously trained model. Use this option to build a new model as a continuation of a previously generated model.
Note: GLM only supports checkpoint for the
IRLSM
solver. The solver option must be set explicitly toIRLSM
and cannot be set toAUTO
. In addition, checkpoint for GLM does not work when crossvalidation is enabled.
early_stopping: Specify whether to stop early when there is no more relative improvement on the training or validation set. This option defaults to
True
(enabled).export_checkpoints_dir: Specify a directory to which generated models will automatically be exported.
fold_assignment: (Applicable only if a value for
nfolds
is specified andfold_column
is not specified) Specify the crossvalidation fold assignment scheme. One of:AUTO
(default; usesRandom
)Random
Modulo
(read more about Modulo)Stratified
(which will stratify the folds based on the response variable for classification problems)
fold_column: Specify the column that contains the crossvalidation fold index assignment per observation.
ignore_const_cols: Enable this option to ignore constant training columns, since no information can be gained from them. This option defaults to
True
(enabled).keep_cross_validation_fold_assignment: Enable this option to preserve the crossvalidation fold assignment. This option defaults to
False
(disabled).keep_cross_validation_models: Specify whether to keep the crossvalidated models. Keeping crossvalidation models may consume significantly more memory in the H2O cluster. This option defaults to
True
(enabled).keep_cross_validation_predictions: Specify whether to keep the crossvalidation predictions. This option defaults to
False
(disabled).max_iterations: Specify the number of training iterations. This options defaults to
1
.max_runtime_secs: Maximum allowed runtime in seconds for model training. Use
0
(default) to disable.missing_values_handling: Specify how to handle missing values. One of:
Skip
,MeanImputation
(default), orPlugValues
.model_id: Specify a custom name for the model to use as a reference. By default, H2O automatically generates a destination key.
nfolds: Specify the number of folds for crossvalidation. The value can be
0
(default) to disable or \(\geq\)2
.offset_column: Specify a column to use as the offset; the value cannot be the same as the value for the
weights_column
.Note: Offsets are perrow “bias values” that are used during model training. For Gaussian distributions, they can be seen as simple corrections to the response (
y
) column. Instead of learning to predict the response (yrow), the model learns to predict the (row) offset of the response column. For other distributions, the offset corrections are applied in the linearized space before applying the inverse link function to get the actual response values.score_each_iteration: Enable this option to score during each iteration of the model training. This option defaults to
False
(disabled).seed: Specify the random number generator (RNG) seed for algorithm components dependent on randomization. The seed is consistent for each H2O instance so that you can create models with the same starting conditions in alternative configurations. This option defaults to
1
(timebased random number).standardize: Specify whether to standardize the numeric columns to have a mean of zero and unit variance. Standardization is highly recommended; if you do not use standardization, the results can include components that are dominated by variables that appear to have larger variances relative to other attributes as a matter of scale, rather than true contribution. This option defaults to
True
(enabled).stopping_metric: Specify the metric to use for early stopping. The available options are:
AUTO
(default): (This defaults tologloss
for classification anddeviance
for regression)deviance
logloss
MSE
RMSE
MAE
RMSLE
AUC
(area under the ROC curve)AUCPR
(area under the PrecisionRecall curve)lift_top_group
misclassification
mean_per_class_error
stopping_rounds: Stops training when the option selected for
stopping_metric
doesn’t improve for the specified number of training rounds, based on a simple moving average. To disable this feature, specify0
(default).Note: If crossvalidation is enabled:
All crossvalidation models stop training when the validation metric doesn’t improve.
The main model runs for the mean number of epochs.
N+1 models may be off by the number specified for
stopping_rounds
from the best model, but the crossvalidation metric estimates the performance of the main model for the resulting number of epochs (which may be fewer than the specified number of epochs).
stopping_tolerance: Specify the relative tolerance for the metricbased stopping to stop training if the improvement is less than this value. Defaults to
0.001
.training_frame: Required Specify the dataset used to build the model. NOTE: In Flow, if you click the Build a model button from the
Parse
cell, the training frame is entered automatically.validation_frame: Specify the dataset used to evaluate the accuracy of the model.
weights_column: Specify a column to use for the observation weights, which are used for bias correction. The specified
weights_column
must be included in the specifiedtraining_frame
.Python only: To use a weights column when passing an H2OFrame to
x
instead of a list of column names, the specifiedtraining_frame
must contain the specifiedweights_column
.Note: Weights are perrow observation weights and do not increase the size of the data frame. This is typically the number of times a row is repeated, but noninteger values are supported as well. During training, rows with higher weights matter more due to the larger loss function prefactor.
x: Specify a vector containing the names or indices of the predictor variables to use when building the model. If
x
is missing, then all columns excepty
are used.y: Required Specify the column to use as the dependent variable.
For a regression model, this column must be numeric (Real or Int).
For a classification model, this column must be categorical (Enum or String). If the family is
Binomial
, the dataset cannot contain more than two levels.
Interpreting a GLM Model¶
By default, the following output displays:
Model parameters (hidden)
A bar chart representing the standardized coefficient magnitudes (blue for negative, orange for positive). Note that this only displays is standardization is enabled.
A graph of the scoring history (objective vs. iteration)
Output (model category, validation metrics, and standardized coefficients magnitude)
GLM model summary (family, link, regularization, number of total predictors, number of active predictors, number of iterations, training frame)
Scoring history in tabular form (timestamp, duration, iteration, log likelihood, objective)
Training metrics (model, model checksum, frame, frame checksum, description, model category, scoring time, predictions, MSE, r2, residual deviance, null deviance, AIC, null degrees of freedom, residual degrees of freedom)
Coefficients
Standardized coefficient magnitudes (if standardization is enabled)
Classification and Regression¶
GLM can produce two categories of models: classification and regression. Logistic regression is the GLM performing binary classification.
Handling of Categorical Variables¶
GLM supports both binary and multinomial classification. For binary classification, the response column can only have two levels; for multinomial classification, the response column will have more than two levels. We recommend letting GLM handle categorical columns, as it can take advantage of the categorical column for better performance and memory utilization.
We strongly recommend avoiding onehot encoding categorical columns with any levels into many binary columns, as this is very inefficient. This is especially true for Python users who are used to expanding their categorical variables manually for other frameworks.
Handling of Numeric Variables¶
When GLM performs regression (with factor columns), one category can be left out to avoid multicollinearity. If regularization is disabled (lambda = 0
), then one category is left out. However, when using a the default lambda parameter, all categories are included.
The reason for the different behavior with regularization is that collinearity is not a problem with regularization. And it’s better to leave regularization to find out which level to ignore (or how to distribute the coefficients between the levels).
Regression Influence Diagnostics¶
Regression influence diagnostics reveal the influence of each data row on the GLM parameter determination for IRLSM. This shows the parameter value change for each predictor when a data row is included and excluded in the dataset used to train the GLM model.
To find the regression diagnostics for the Gaussian family, the output is:
For the whole dataset, there is:
where:
\(Y\) is a column vector with \(N\) elements and \(Y = \begin{bmatrix} y_0 \\ y_1 \\ y_2 \\ \vdots \\ y_{N1} \\\end{bmatrix}\);
\(X\) is a \(N \times p\) matrix containing \(X = \begin{bmatrix} x_0^T \\ x_1^T \\ x_2^T \\ \vdots \\ x_{N1}^T \\\end{bmatrix}\);
\(x_i\) is a column vector with \(p\) elements: \(x_i = \begin{bmatrix} x_{i0} \\ x_{i1} \\ \vdots \\ x_{ip 2} \\ 1 \\\end{bmatrix}\) where \(1\) is added to represent the term associated with the intercept term.
The least square solution for \(\beta\) is:
The residual is defined as:
The projection matrix is:
The residual in equation 1 is good at pointing out illfitting points. However, if does not adequately reveal which observations unduly influence the fit of \(\beta\). The diagonal of \(M\) can direct to those points. Influential points tend to have small values of \(m_{ii}\) (much smaller than the average value of \(1  \frac{m}{N}\) where \(m\) is the number of predictors and \(N\) is the number of rows of data in the dataset).
The GLM model is then fitted with all the data to find \(\hat{\beta}\). Data row \(l\) is then deleted and the GLM model is fitted again to find \(\hat{\beta}(l)\) as the model coefficients. The influence of data row \(l\) can be found by looking at the parameter value change:
The DFBETAS for the \(k\text{th}\) coefficient due to the absence of data row \(l\) is calculated as:
where:
\(s_{(l)}^2 = \frac{1}{N1p} \sum_{i = 0 \text{ & } i \neq l}^{N1} \big( y_i  x_i^T \hat{\beta}(l) \big)^2\) is for a nonweighted dataset. We have implemented the version of \(s_{(l)}^2\) that works with both weighted and nonweighted datasets.
\((X^TX)_{kk}^{1}\) is the diagonal of the gram matrix inverse.
To find the regression diagnostics for the Binomial family, the output is
where \(\mu_i = \frac{1}{1 + exp( \beta^T x_i \beta_0)}\) and \(y_i = 1 \text{ or } 0\). The iterative coefficient update can be written as:
where:
\(V\) is a diagonal matrix with diagonal value \(v_{ii} = \mu_i (1\mu_i)\);
\(s_i = y_i  \mu_i\).
The formula for DFBETAS for the \(k\text{th}\) coefficient due to the ansence of data row \(l\) is defined as:
where:
\(\hat{\sigma}_k\) is the standard error of the \(k\text{th}\) coefficient;
\(\Delta_l \hat{\beta}_k\) is the \(k\text{th}\) element of the vector \(\Delta_l \hat{\beta}\) which is approximated as:
\(w_l\) is the weight assigned to the data row;
\(h_{ll}\) is the diagonal of a hat matrix which is calculated as:
Family and Link Functions¶
GLM problems consist of three main components:
A random component \(f\) for the dependent variable \(y\): The density function \(f(y;\theta,\phi)\) has a probability distribution from the exponential family parametrized by \(\theta\) and \(\phi\). This removes the restriction on the distribution of the error and allows for nonhomogeneity of the variance with respect to the mean vector.
A systematic component (linear model) \(\eta\): \(\eta = X\beta\), where \(X\) is the matrix of all observation vectors \(x_i\).
A link function \(g\): \(E(y) = \mu = {g^1}(\eta)\) relates the expected value of the response \(\mu\) to the linear component \(\eta\). The link function can be any monotonic differentiable function. This relaxes the constraints on the additivity of the covariates, and it allows the response to belong to a restricted range of values depending on the chosen transformation \(g\).
Accordingly, in order to specify a GLM problem, you must choose a family function \(f\), link function \(g\), and any parameters needed to train the model.
Families¶
The family
option specifies a probability distribution from an exponential family. You can specify one of the following, based on the response column type:
gaussian
: (See Linear Regression (Gaussian Family).) The response must be numeric (Real or Int). This is the default family.binomial
: (See Logistic Regression (Binomial Family)). The response must be categorical 2 levels/classes or binary (Enum or Int).fractionalbinomial
: See (Fractional Logit Model (Fraction Binomial)). The response must be a numeric between 0 and 1.ordinal
: (See Logistic Ordinal Regression (Ordinal Family)). Requires a categorical response with at least 3 levels. (For 2class problems, use family=”binomial”.)quasibinomial
: (See PseudoLogistic Regression (Quasibinomial Family)). The response must be numeric.multinomial
: (See Multiclass Classification (Multinomial Family)). The response can be categorical with more than two levels/classes (Enum).poisson
: (See Poisson Models). The response must be numeric and nonnegative (Int).gamma
: (See Gamma Models). The response must be numeric and continuous and positive (Real or Int).tweedie
: (See Tweedie Models). The response must be numeric and continuous (Real) and nonnegative.negativebinomial
: (See Negative Binomial Models). The response must be numeric and nonnegative (Int).AUTO
: Determines the family automatically for the user.
Note: If your response column is binomial, then you must convert that column to a categorical (.asfactor()
in Python and as.factor()
in R) and set family = binomial
. The following configurations can lead to unexpected results.
If you DO convert the response column to categorical and DO NOT to set
family=binomial
, then you will receive an error message.If you DO NOT convert response column to categorical and DO NOT set the family, then GLM will assume the 0s and 1s are numbers and will provide a Gaussian solution to a regression problem.
Linear Regression (Gaussian Family)¶
Linear regression corresponds to the Gaussian family model. The link function \(g\) is the identity, and density \(f\) corresponds to a normal distribution. It is the simplest example of a GLM but has many uses and several advantages over other families. Specifically, it is faster and requires more stable computations. Gaussian models the dependency between a response \(y\) and a covariates vector \(x\) as a linear function:
The model is fitted by solving the least squares problem, which is equivalent to maximizing the likelihood for the Gaussian family.
The deviance is the sum of the squared prediction errors:
Logistic Regression (Binomial Family)¶
Logistic regression is used for binary classification problems where the response is a categorical variable with two levels. It models the probability of an observation belonging to an output category given the data (for example, \(Pr(y=1x)\)). The canonical link for the binomial family is the logit function (also known as log odds). Its inverse is the logistic function, which takes any real number and projects it onto the [0,1] range as desired to model the probability of belonging to a class. The corresponding scurve is below:
The fitted model has the form:
This can alternatively be written as:
The model is fitted by maximizing the following penalized likelihood:
The corresponding deviance is equal to:
Fractional Logit Model (Fraction Binomial)¶
In the financial service industry, there are many outcomes that are fractional in the range of [0,1]. For example, LGD (Loss Given Default in credit risk) measures the proportion of losses not recovered from a default borrower during the collection process, and this can be observed to be in the closed interval [0, 1]. The following assumptions are made for this model.
\(\text{Pr}(y=1x) = E(y) = \frac{1}{1 + \text{exp}(\beta^T x\beta_0)}\)
The likelihood function = \(\text{Pr}{(y=1x)}^y (1\text{Pr}(y=1x))^{(1y)}\) for \(1 \geq y \geq 0\)
\(var(y) = \varphi E(y)(1E(y))\) and \(\varphi\) is estimated as \(\varphi = \frac{1}{np} \frac{\sum {(y_i  E(y))}2} {E(y)(1E(y))}\)
Note that these are exactly the same as the binomial distribution. However, the values are calculated with the value of \(y\) in the range of 0 and 1 instead of just 0 and 1. Therefore, we implemented the fractional binomial family using the code of binomial. Changes are made when needed.
Logistic Ordinal Regression (Ordinal Family)¶
A logistic ordinal regression model is a generalized linear model that predicts ordinal variables  variables that are discreet, as in classification, but that can be ordered, as in regression.
Let \(X_i\in\rm \Bbb I \!\Bbb R^p\), \(y\) can belong to any of the \(K\) classes. In logistic ordinal regression, we model the cumulative distribution function (CDF) of \(y\) belonging to class \(j\), given \(X_i\) as the logistic function:
Compared to multiclass logistic regression, all classes share the same \(\beta\) vector. This adds the constraint that the hyperplanes that separate the different classes are parallel for all classes. To decide which class will \(X_i\) be predicted, we use the thresholds vector \(\theta\). If there are \(K\) different classes, then \(\theta\) is a nondecreasing vector (that is, \(\theta_0 \leq \theta_1 \leq \ldots \theta_{K2})\) of size \(K1\). We then assign \(X_i\) to the class \(j\) if \(\beta^{T}X_i + \theta_j > 0\) for the lowest class label \(j\).
We choose a logistic function to model the probability \(P(y \leq jX_i)\) but other choices are possible.
To determine the values of \(\beta\) and \(\theta\), we maximize the loglikelihood minus the same Regularization Penalty, as with the other families. However, in the actual H2O3 code, we determine the values of \(\alpha\) and \(\theta\) by minimizing the negative loglikelihood plus the same Regularization Penalty.
Conventional ordinal regression uses a likelihood function to adjust the model parameters. However, during prediction, GLM looks at the log CDF odds.
As a result, there is a small disconnect between the two. To remedy this, we have implemented a new algorithm to set and adjust the model parameters.
Recall that during prediction, a dataset row represented by \(X_i\) will be set to class \(j\) if
and
Hence, for each training data sample \((X_{i}, y_i)\), we adjust the model parameters \(\beta, \theta_0, \theta_1, \ldots, \theta_{K2}\) by considering the thresholds \(\beta^{T}X_i + \theta_j\) directly. The following loss function is used to adjust the model parameters:
Again, you can add the Regularization Penalty to the loss function. The model parameters are adjusted by minimizing the loss function using gradient descent. When the Ordinal family is specified, the solver
parameter will automatically be set to GRADIENT_DESCENT_LH
and use the loglikelihood function. To adjust the model parameters using the loss function, you can set the solver parameter to GRADIENT_DESCENT_SQERR
.
Because only firstorder methods are used in adjusting the model parameters, use Grid Search to choose the best combination of the obj_reg
, alpha
, and lambda
parameters.
In general, the loss function methods tend to generate better accuracies than the likelihood method. In addition, the loss function method is faster as it does not deal with logistic functions  just linear functions when adjusting the model parameters.
PseudoLogistic Regression (Quasibinomial Family)¶
The quasibinomial family option works in the same way as the aforementioned binomial family. The difference is that binomial models only support 0/1 for the values of the target. A quasibinomial model supports “pseudo” logistic regression and allows for two arbitrary integer values (for example 4, 7). Additional information about the quasibinomial option can be found in the “Estimating Effects on Rare Outcomes: Knowledge is Power” paper.
Multiclass Classification (Multinomial Family)¶
Multinomial family generalization of the binomial model is used for multiclass response variables. Similar to the binomail family, GLM models the conditional probability of observing class “c” given “x”. A vector of coefficients exists for each of the output classes. (\(\beta\) is a matrix.) The probabilities are defined as:
The penalized negative loglikelihood is defined as:
where \(\beta_c\) is a vector of coefficients for class “c”, and \(y_{i,k}\) is the \(k\text{th}\) element of the binary vector produced by expanding the response variable using onehot encoding (i.e., \(y_{i,k} == 1\) iff the response at the \(i\text{th}\) observation is “k”; otherwise it is 0.)
Poisson Models¶
Poisson regression is typically used for datasets where the response represents counts, and the errors are assumed to have a Poisson distribution. In general, it can be applied to any data where the response is nonnegative. It models the dependency between the response and covariates as:
The model is fitted by maximizing the corresponding penalized likelihood:
The corresponding deviance is equal to:
Note in the equation above that H2O3 uses the negative log of the likelihood. This is different than the way deviance is specified in https://onlinecourses.science.psu.edu/stat501/node/377/. In order to use this deviance definition, simply multiply the H2O3 deviance by 1.
Gamma Models¶
The gamma distribution is useful for modeling a positive continuous response variable, where the conditional variance of the response grows with its mean, but the coefficientof variation of the response \(\sigma^2(y_i)/\mu_i\) is constant. It is usually used with the log link \(g(\mu_i) = \text{log}(\mu_i)\) or the inverse link \(g(\mu_i) = \dfrac {1} {\mu_i}\), which is equivalent to the canonical link.
The model is fitted by solving the following likelihood maximization:
The corresponding deviance is equal to:
Tweedie Models¶
Tweedie distributions are a family of distributions that include gamma, normal, Poisson, and their combinations. Tweedie distributions are especially useful for modeling positive continuous variables with exact zeros. The variance of the Tweedie distribution is proportional to the \(p\){th} power of the mean \(var(y_i) = \phi\mu{^p_i}\), where \(\phi\) is the dispersion parameter and \(p\) is the variance power.
The Tweedie distribution is parametrized by variance power \(p\) while \(\phi\) is an unknown constant. It is defined for all \(p\) values except in the (0,1) interval and has the following distributions as special cases:
\(p = 0\): Normal
\(p = 1\): Poisson
\(p \in (1,2)\): Compound Poisson, nonnegative with mass at zero
\(p = 2\): Gamma
\(p = 3\): InverseGaussian
\(p > 2\): Stable, with support on the positive reals
The model likelood to maximize has the form:
where the function \(a(y_i,\phi)\) is evaluated using an infinite series expansion and does not have an analytical solution. However, because \(\phi\) is an unknown constant, \(\sum_{i=1}^N\text{log}(a(y_i,\phi))\) is a constant and will be ignored. Hence, the final objective function to minimize with the penalty term is:
The link function in the GLM representation of the Tweedie distribution defaults to:
And \(q = 1  p\). The link power \(q\) can be set to other values as well.
The corresponding deviance is equal to:
Negative Binomial Models¶
Negative binomial regression is a generalization of Poisson regression that loosens the restrictive assumption that the variance is equal to the mean. Instead, the variance of negative binomial is a function of its mean and parameter \(\theta\), the dispersion parameter.
Let \(Y\) denote a random variable with negative binomial distribution, and let \(\mu\) be the mean. The variance of \(Y (\sigma^2)\) will be \(\sigma^2 = \mu + \theta\mu^2\). The possible values of \(Y\) are nonnegative integers like 0, 1, 2, …
The negative binomial regression for an observation \(i\) is:
where \(\Gamma(x)\) is the gamma function, and \(\mu_i\) can be modeled as:
The negative log likelihood \(L(y_i,\mu_i)\) function is:
The final penalized negative log likelihood is used to find the coefficients \(\beta, \beta_0\) given a fixed \(\theta\) value:
The corresponding deviance is:
Note: Future versions of this model will optimize the coefficients as well as the dispersion parameter. Please stay tuned.
Links¶
As indicated previously, a link function \(g\): \(E(y) = \mu = {g^1}(\eta)\) relates the expected value of the response \(\mu\) to the linear component \(\eta\). The link function can be any monotonic differentiable function. This relaxes the constraints on the additivity of the covariates, and it allows the response to belong to a restricted range of values depending on the chosen transformation \(g\).
H2O’s GLM supports the following link functions: Family_Default, Identity, Logit, Log, Inverse, Tweedie, and Ologit.
The following table describes the allowed Family/Link combinations.
Family 
Link Function 

Family_Default 
Identity 
Logit 
Log 
Inverse 
Tweedie 
Ologit 

Binomial 
X 
X 

Fractional Binomial 
X 
X 

Quasibinomial 
X 
X 

Multinomial 
X 

Ordinal 
X 
X 

Gaussian 
X 
X 
X 
X 

Poisson 
X 
X 
X 

Gamma 
X 
X 
X 
X 

Tweedie 
X 
X 

Negative Binomial 
X 
X 
X 

AUTO 
X*** 
X* 
X** 
X* 
X* 
For AUTO:
X*: the data is numeric (
Real
orInt
) (family determined asgaussian
)X**: the data is
Enum
with cardinality = 2 (family determined asbinomial
)X***: the data is
Enum
with cardinality > 2 (family determined asmultinomial
)
Dispersion Parameter Estimation¶
Regularization is not supported when you use dispersion parameter estimation with maximum likelihood.
Tweedie¶
The density for the maximum likelihood function for Tweedie can be written as:
where:
\(a (y, \phi, p), k(\theta)\) are suitable known functions
\(\phi\) is the dispersion parameter and is positive
\(\theta = \begin{cases} \frac{\mu ^{1p}}{1p} & p \neq 1 \\ \log (\mu) & p = 1 \\\end{cases}\)
\(k(\theta) = \begin{cases} \frac{\mu ^{2p}}{2p} & p \neq 2 \\ \log (\mu) & p=2 \\\end{cases}\)
the value of \(\alpha (y,\phi)\) depends on the value of \(p\)
If there are weights introduced to each data row, equation 1 will become:
\(\alpha (y,\phi)\) when \(1 < p < 2\)¶
For \(Y=0\),
For \(Y>0\),
with \(W(y, \phi, p) = \sum^{\infty}_{j=1} W_j\) and
If weight is applied to each row, equation 4 becomes:
The \(W_j\) terms are all positive. The following figure plots for \(\mu = 0.5, p=1.5, \phi =1. y=0.1\).
\(\alpha (y,\phi)\) when \(p > 2\)¶
Here, you have
and \(V = \sum^{\infty}_{k=1} V_k\) where
Note that \(0 < \alpha < 1\) for \(p>2\). The \(V_k\) terms are both positive and negative. This will limit the numerical accuracy that is obtained in summing it as shown in the following image. Again, if weights are applied to each row of the dataset, equation 6 becomes:
In the following figure, we use \(\mu =0.5,p=2.5,\phi =1, y=0.1\).
Warnings¶
Accuracy and Limitation
While the Tweedie’s probability density function contains an infinite series sum, when \(p\) is close to 2, the response (\(y\)) is large, and \(\phi\) is small the common number of terms that are needed to approximate the infinite sum grow without bound. This causes an increase in computation time without reaching the desired accuracy.
Multimodal Densities
As \(p\) closes in on 1, the Tweedie density function becomes multimodal. This means that the optimization procedure will fail since it will not be able to find the global optimal point. It will instead arrive at a local optimal point.
As a conservative condition, to ensure that the density is unimodal for most values of \(y,\phi\), we should have \(p>1.2\).
Tweedie Dispersion Example¶
# Import the training data:
training_data < h2o.importFile("http://h2opublictestdata.s3.amazonaws.com/smalldata/glm_test/tweedie_p3_phi1_10KRows.csv")
# Set the predictors and response:
predictors < c('abs.C1.', 'abs.C2.', 'abs.C3.', 'abs.C4.', 'abs.C5.')
response < 'x'
# Build and train the model:
model < h2o.glm(x = predictors,
y = response,
training_frame = training_data,
family = 'tweedie',
tweedie_variance_power = 3,
lambda = 0,
compute_p_values = TRUE,
dispersion_parameter_method = "pearson",
init_dispersion_parameter = 0.5,
dispersion_epsilon = 1e4,
max_iterations_dispersion = 100)
# Retrieve the estimated dispersion:
model@model$dispersion
[1] 0.7599965
# Import the training data:
training_data = h2o.import_file("http://h2opublictestdata.s3.amazonaws.com/smalldata/glm_test/tweedie_p3_phi1_10KRows.csv")
# Set the predictors and response:
predictors = ["abs.C1.", "abs.C2.", "abs.C3.", "abs.C4.", "abs.C5.""]
response = "x"
# Build and train the model:
model = H2OGeneralizedLinearEstimator(family="tweedie",
lambda_=0,
compute_p_values=True,
dispersion_parameter_method="pearson",
init_dispersion_parameter=0.5,
dispersion_epsilon=1e4,
tweedie_variance_power=3,
max_iterations_dispersion=100)
model.train(x=predictors, y=response, training_frame=training_data)
# Retrieve the estimated dispersion:
model._model_json["output"]["dispersion"]
0.7599964835351135
Negative Binomial¶
GLM dispersion estimation using the maximum likelihood method for the negative binomial family is available when you set dispersion_parameter_method=“ml”
.
The coefficients, or betas, are estimated using IRLSM. The dispersion parameter theta is estimated after each IRLSM iteration. After the first beta update, the initial theta estimate is made using the method of moments as a starting point. Then, theta is updated using the maximum likelihood in each iteration.
While not converged:
Estimate coefficients (betas)
Estimate dispersion (theta)
If it is the first iteration:
Theta \(\gets\) Method of Moments estimate
Otherwise:
Theta \(\gets\) Maximum Likelihood estimate using Newton’s method with learning rate estimated using Golden section search
Hierarchical GLM¶
Introduced in 3.28.0.1, Hierarchical GLM (HGLM) fits generalized linear models with random effects, where the random effect can come from a conjugate exponentialfamily distribution (for example, Gaussian). HGLM allows you to specify both fixed and random effects, which allows fitting correlated to random effects as well as random regression models. HGLM can be used for linear mixed models and for generalized linear mixed models with random effects for a variety of links and a variety of distributions for both the outcomes and the random effects.
Note: The initial release of HGLM supports only the Gaussian family and random family.
Gaussian Family and Random Family in HGLM¶
To build an HGLM, we need the hierarchical loglikelihood (hlikelihood) function. The hlikelihood function can be expressed as (equation 1):
for fixed effects \(\beta\), variance components \(\theta\), and random effects \(u\).
A standard linar mixed model can be expressed as (equation 2):
where
\(e \text ~ N(0, I_n, \delta_e^2), u \text ~ N(0, I_k, \delta_u^2)\)
\(e, u\) are independent, and \(u\) represents the random effects
\(n\) is the number of i.i.d observations of \(y\) with mean \(0\)
\(q\) is the number of values \(Z\) can take
Then rewriting equation 2 as \(e = X\beta + Zu  y\) and derive the hlikelihood as:
where \(C_1 =  \frac{n}{2} \log(2\pi), C_2 =  \frac{q}{2} \log(2\pi)\)
In principal, the HGLM model building involves the following main steps:
Set the initial values to \(\delta_u^2, \delta_e^2, u, \beta\)
Estimate the fixed (\(\beta\)) and random effects (\(u\)) by solving for \(\frac{\partial h}{\partial \beta} = 0, \frac{\partial h}{\partial u} = 0\)
Estimate variance components using the adjusted profile likelihood:
\[h_p = \big(h + \frac{1}{2} log \big 2 \pi D^{1}\big \big)_{\beta=\hat \beta, u=\hat u}\]and solving for
\[\frac{\partial h_p}{\partial \theta} = 0\]Note that \(D\) is the matrix of the second derivatives of \(h\) around \(\beta = \hat \beta, u = \hat u, \theta = (\delta_u^2, \delta_e^2)\).
H2O Implementation¶
In reality, Lee and Nelder (see References) showed that linear mixed models can be fitted using a hierarchy of GLM by using an augmented linear model. The linear mixed model will be written as:
where \(R\) is a diagonal matrix with elements given by the estimated dispersion model. The dispersion model refers to the variance part of the fixed effect model with error \(e\). There are cases where the dispersion model is modeled itself as \(exp(x_d, \beta_d)\). However, in our current version, the variance is just a constant \(\sigma_e^2\), and hence \(R\) is just a scalar value. It is initialized to be the identity matrix. The model can be written as an augmented weighted linear model:
where
Note that \(q\) is the number of columns in \(Z, 0_q\) is a vector of \(q\) zeroes, \(I_q\) is the \(qxq\) identity matrix. The variancecovariance matrix of the augmented residual matrix is
Fixed and Random Coefficients Estimation¶
The estimates for \(\delta\) from weighted least squares are given by solving
where
The two variance components are estimated iteratively by applying a gamma GLM to the residuals \(e_i^2,u_i^2\). Because we are not using a dispersion model, there is only an intercept terms in the linear predictors. The leverages \(h_i\) for these models are calculated from the diagonal elements of the hat matrix:
Estimation of Fixed Effect Dispersion Parameter/Variance¶
A gamma GLM is used to fit the dispersion part of the model with response \(y_{d,i}=(e_i^2)⁄(1h_i )\) where \(E(y_d )=u_d\) and \(u_d≡\phi\) (i.e., \(\delta_e^2\) for a Gaussian response). The GLM model for the dispersion parameter is then specified by the link function \(g_d (.)\) and the linear predictor \(X_d \beta_d\) with prior weights for \((1h_i )⁄2\) for \(g_d (u_d )=X_d \beta_d\). Because we are not using a dispersion model, \(X_d \beta_d\) will only contain the intercept term.
Estimation of Random Effect Dispersion Parameter/Variance¶
Similarly, a gamma GLM is fitted to the dispersion term \(alpha\) (i.e., \(\delta_e^2\) for a GLM) for the random effect \(v\), with \(y_\alpha,j = u_j^2⁄(1h_{n+j}), j=1,2,…,q\) and \(g_\alpha (u_\alpha )=\lambda\), where the prior weights are \((1h_{n+j} )⁄2\), and the estimated dispersion term for the random effect is given by \(\hat \alpha = g_α^{1}(\hat \lambda)\).
Fitting Algorithm Overview¶
The following fitting algorithm from “Generalized linear models with random effects” (Y. Lee, J. A. Nelder and Y. Pawitan; see References) is used to build our HGLM. Let \(n\) be the number of observations and \(k\) be the number of levels in the random effect. The algorithm that was implemented here at H2O will perform the following:
Initialize starting values either from user by setting parameter startval or by the system if startval is left unspecified.
Construct an augmented model with response \(y_{aug}= {y \choose {E(u)}}\).
Use a GLM to estimate \(\delta={\beta \choose u}\) given the dispersion \(\phi\) and \(\lambda\). Save the deviance components and leverages from the fitted model.
Use a gamma GLM to estimate the dispersion parameter for \(\phi\) (i.e. \(\delta_e^2\) for a Gaussian response).
Use a similar GLM as in step 4 to estimate \(\lambda\) from the last \(k\) deviance components and leverages obtained from the GLM in step 3.
Iterate between steps 35 until convergence. Note that the convergence measure here is either a timeout event or the following condition has been met: \(\frac {\Sigma_i{(\text{eta}. i  \text{eta}.o)^2}} {\Sigma_i(\text{eta}.i)^2 \text{<} 1e  6}\).
A timeout event can be defined as the following:
Maximum number of iterations have been reached
Model building run time exceeds what is specified in
max_runtime_secs
A user has clicked on stop model button or similar from Flow.
For families and random families other than Gaussian, link functions are used to translate from the linear space to the model the mean output.
HGLM Model Metrics¶
H2O provides the following model metrics at the end of each HGLM experiment:
fixef: fixed effects coefficients
ranef: random effects coefficients
randc: vector of random column indices
varfix: dispersion parameter of the mean model
varranef: dispersion parameter of the random effects
converge: true if algorithm has converge, otherwise false
sefe: standard errors of fixed effects
sere: standard errors of random effects
dfrefe: deviance degrees of freedom for the mean part of model
sumvc1: estimates and standard errors of linear predictor in the dispersion model
summvc2: estimates and standard errors of the linear predictor for the dispersion parameter of the random effects
likelihood: if
calc_like
is true, the following four values are returned:hlik: loghlikelihood;
pvh: adjusted profile loglikelihood profiled over the random effects;
pbvh: adjusted profile loglikelihood profiled over fixed and random effects;
caic: conditional AIC.
bad: row index of the most influential observation.
Mapping of Fitting Algorithm to the H2O3 Implementation¶
This mapping is done in four steps:
Initialize starting values by the system.
Estimate \(\delta =\) \(\beta \choose u\).
Estimate \(\delta_e^2(\text {tau})\).
Estimate \(\delta_u^2(\text {phi})\).
Step 1: Initialize starting values by the system.
Following the implementation from R, when a user fails to specify starting values for psi, \(\beta\), \(\mu\), \(\delta_e^2\), \(\delta_u^2\), we will do it for the users as follows:
A GLM model is built with just the fixed columns and response.
Next init_sig_e(\(\delta_e^2\))/tau is set to 0.6*residual_deviance()/residual_degrees_of_freedom().
init_sig_u(\(\delta_u^2\)) is set to 0.66*init_sig_e.
For numerical stability, we restrict the magnitude to init_sig_e and init_sig_u to >= 0.1.
Set phi = vector of length number of random columns of value init_sig_u/(number of random columns).
Set \(\beta\) to the GLM model coefficients, \(\mu\) to be a zero vector.
Set psi to be a zero vector.
Step 2: Estimate \(\delta =\) \(\beta \choose u\).
Given the current values of \(\delta_e^2, \delta_u^2\), we will solve for \(\delta =\) \(\beta \choose u\). Instead of solving \(\delta\) from \(T_a^T W^{1} T_a \delta=T_a^T W^{1} y_a\), a different set of formulae are used. A loop is used to solve for the coefficients:
The following variables are generated:
\(v.i= g_r^{1} (u_i)\) where \(u_i\) are the random coefficients of the random effects/columns and \(g_r^{1}\) can be considered as the inverse link function.
\(tau\) is a vector of length number of data containing init.sig.e;
\(eta.i=X_i \beta+offset\) and store the previous \(eta.i\) as \(eta.o\).
\(mu.i=g^{1} (eta.i)\).
dmu_deta is derivative of \(g^{1} (eta.i)\) with respect to \(eta.i\), which is 1 for identity link.
\(z_i=eta.ioffset+(y_imu.i)/\text {dmu_deta}\)
\(zmi= \text{psi}\)
\(augZ =\) \(zi \choose zmi\).
du_dv is the derivative of \(g_r^{1} (u_i)\) with respect to \(v.i.\) Again, for identity link, this is 1.
The weight \(W =\) \(wdata \choose wpsi\) where \(wdata = \frac {d \text{mu_deta}^2}{\text {prior_weight*family}\$\text{variance}(mu.i)*tau}\) and \(wpsi = \frac {d \text{u_dv}^2}{\text {prior_weight*family}\$\text{variance(psi)*phi}}\)
Finally the following formula is used to solve for the parameters: \(augXZ \cdot \delta=augZW\) where \(augXZ=T_a \cdot W\) and \(augZW=augZ \cdot W\):
Use QR decomposition to augXZ and obtain: \(QR \delta = augZW\).
Use backward solve to obtain the coefficients \(\delta\) from \(R \delta = Q^T augZW\).
Calculate \(hv=\text{rowsum}(Q)\) of length n+number of expanded and store in returnFrame.
Calculate \(dev =\) \(prior weight*(y_imu.i)^2 \choose (psi u_i )^2\) of length n+number of expanded random columns and store in returnFrame.
Calculate \(resid= \frac {(ymu.i)} {\sqrt \frac {sum(dev)(1hv)}{np}}\) of length n and store in returnFrame.
Go back to step 1 unless \(\Sigma_i(eta.ieta.o)^2 / \Sigma_i(eta.i)^2<1e6\) or a timeout event has occurred.
Step 3: Estimate \(\delta_e^2(\text {tau})\)
With the newly estimated fixed and random coefficients, we will estimate the dispersion parameter for the fixed effects/columns by building a gamma GLM:
Generate a training frame with constant predictor column of 1 to force glm model to generate only the intercept term:
Response column as \(dev/(1hv)\).
Weight column as \((1hv)/2\).
Predictor column of ones.
The length of the training frame is the number of data rows.
Build a gamma GLM with
family=gamma
andlink=log
.Set \(tau = \text {exp (intercept value)}\).
Assign estimation standard error and sigma from the GLM standard error calculation for coefficients.
Step 4: Estimate \(\delta_u^2(\text {phi})\).
Again, a gamma GLM model is used here. In addition, the error estimates are generated for each random column. Exactly the same steps are used here as in Step 3. The only difference is that we are looking at the \(dev,hv\) corresponding to the expanded random columns/effects.
Regularization¶
Regularization is used to attempt to solve problems with overfitting that can occur in GLM. Penalties can be introduced to the model building process to avoid overfitting, to reduce variance of the prediction error, and to handle correlated predictors. The two most common penalized models are ridge regression and LASSO (least absolute shrinkage and selection operator). The elastic net combines both penalties using both the alpha
and lambda
options (i.e., values greater than 0 for both).
LASSO and Ridge Regression¶
LASSO represents the \(\ell{_1}\) penalty and is an alternative regularized least squares method that penalizes the sum of the absolute coefficents \(\beta{_1} = \sum{^p_{k=1}} \beta{^2_k}\). LASSO leads to a sparse solution when the tuning parameter is sufficiently large. As the tuning parameter value \(\lambda\) is increased, all coefficients are set to zero. Because reducing parameters to zero removes them from the model, LASSO is a good selection tool.
Ridge regression penalizes the \(\ell{_2}\) norm of the model coefficients \(\beta{^2_2} = \sum{^p_{k=1}} \beta{^2_k}\). It provides greater numerical stability and is easier and faster to compute than LASSO. It keeps all the predictors in the model and shrinks them proportionally. Ridge regression reduces coefficient values simultaneously as the penalty is increased without setting any of them to zero.
Variable selection is important in numerous modern applications wiht many covariates where the \(\ell{_1}\) penalty has proven to be successful. Therefore, if the number of variables is large or if the solution is known to be sparse, we recommend using LASSO, which will select a small number of variables for sufficiently high \(\lambda\) that could be crucial to the inperpretability of the mode. The \(\ell{_2}\) norm does not have this effect; it shrinks the coefficients but does not set them exactly to zero.
The two penalites also differ in the presence of correlated predictors. The \(\ell{_2}\) penalty shrinks coefficients for correlated columns toward each other, while the \(\ell{_1}\) penalty tends to select only one of them and sets the other coefficients to zero. Using the elastic net argument \(\alpha\) combines these two behaviors.
The elastic net method selects variables and preserves the grouping effect (shrinking coefficients of correlated columns together). Moreover, while the number of predictors that can enter a LASSO model saturates at min \((n,p)\) (where \(n\) is the number of observations, and \(p\) is the number of variables in the model), the elastic net does not have this limitation and can fit models with a larger number of predictors.
Elastic Net Penalty¶
As indicated previously, elastic net regularization is a combination of the \(\ell{_1}\) and \(\ell{_2}\) penalties parametrized by the \(\alpha\) and \(\lambda\) arguments (similar to “Regularization Paths for Genarlized Linear Models via Coordinate Descent” by Friedman et all).
\(\alpha\) controls the elastic net penalty distribution between the \(\ell_1\) and \(\ell_2\) norms. It can have any value in the [0,1] range or a vector of values (via grid search). If \(\alpha=0\), then H2O solves the GLM using ridge regression. If \(\alpha=1\), then LASSO penalty is used.
\(\lambda\) controls the penalty strength. The range is any positive value or a vector of values (via grid search). Note that \(\lambda\) values are capped at \(\lambda_{max}\), which is the smallest \(\lambda\) for which the solution is all zeros (except for the intercept term).
The combination of the \(\ell_1\) and \(\ell_2\) penalties is beneficial because \(\ell_1\) induces sparsity, while \(\ell_2\) gives stability and encourages the grouping effect (where a group of correlated variables tend to be dropped or added into the model simultaneously). When focusing on sparsity, one possible use of the \(\alpha\) argument involves using the \(\ell_1\) mainly with very little \(\ell_2\) (\(\alpha\) almost 1) to stabilize the computation and improve convergence speed.
Regularization Parameters in GLM¶
To get the best possible model, we need to find the optimal values of the regularization parameters \(\alpha\) and \(\lambda\). To find the optimal values, H2O allows you to perform a grid search over \(\alpha\) and a special form of grid search called “lambda search” over \(\lambda\).
The recommended way to find optimal regularization settings on H2O is to do a grid search over a few \(\alpha\) values with an automatic lambda search for each \(\alpha\).
Alpha
The
alpha
parameter controls the distribution between the \(\ell{_1}\) (LASSO) and \(\ell{_2}\) (ridge regression) penalties. A value of 1.0 foralpha
represents LASSO, and analpha
value of 0.0 produces ridge reguression.
Lambda
The
lambda
parameter controls the amount of regularization applied. Iflambda
is 0.0, no regularization is applied, and thealpha
parameter is ignored. The default value forlambda
is calculated by H2O using a heuristic based on the training data. If you allow H2O to calculate the value forlambda
, you can see the chosen value in the model output.
Lambda Search¶
If the lambda_search
option is set, GLM will compute models for full regularization path similar to glmnet. (See the glmnet paper.) Regularization path starts at lambda max (highest lambda values which makes sense  i.e. lowest value driving all coefficients to zero) and goes down to lambda min on log scale, decreasing regularization strength at each step. The returned model will have coefficients corresponding to the “optimal” lambda value as decided during training.
When looking for a sparse solution (alpha
> 0), lambda search can also be used to efficiently handle very wide datasets because it can filter out inactive predictors (noise) and only build models for a small subset of predictors. A possible use case for lambda search is to run it on a dataset with many predictors but limit the number of active predictors to a relatively small value.
Lambda search can be configured along with the following arguments:
alpha
: Regularization distribution between \(\ell_1\) and \(\ell_2\).validation_frame
and/ornfolds
: Used to select the best lambda based on the crossvalidation performance or the validation or training data. If available, crossvalidation performance takes precedence. If no validation data is available, the best lambda is selected based on training data performance and is therefore guaranteed to always be the minimal lambda computed since GLM cannot overfit on a training dataset.
Note: If running lambda search with a validation dataset and crossvalidation disabled, the chosen lambda value corresponds to the lambda with the lowest validation error. The validation dataset is used to select the model, and the model performance should be evaluated on another independent test dataset.
lambda_min_ratio
andnlambdas
: The sequence of the \(\lambda\) values is automatically generated as an exponentially decreasing sequence. It ranges from \(\lambda_{max}\) (the smallest \(\lambda\) so that the solution is a model with all 0s) to \(\lambda_{min} =\)lambda_min_ratio
\(\times\) \(\lambda_{max}\).
H2O computes \(\lambda\) models sequentially and in decreasing order, warmstarting the model (using the previous solutin as the initial prediction) for \(\lambda_k\) with the solution for \(\lambda_{k1}\). By warmstarting the models, we get better performance. Typically models for subsequent \(\lambda\) values are close to each other, so only a few iterations per \(\lambda\) are needed (two or three). This also achieves greater numerical stability because models with a higher penalty are easier to compute. This method starts with an easy problem and then continues to make small adjustments.
Note:
lambda_min_ratio
andnlambdas
also specify the relative distance of any two lambdas in the sequence. This is important when applying recursive strong rules, which are only effective if the neighboring lambdas are “close” to each other. The default value forlambda_min_ratio
is \(1e^{4}\), and the default value fornlambdas
is 100. This gives a ratio of 0.912. For best results when using strong rules, keep the ratio close to this default.
max_active_predictors
: This limits the number of active predictors. (The actual number of nonzero predictors in the model is going to be slightly lower.) It is useful when obtaining a sparse solution to avoid costly computation of models with too many predictors.
Full Regularization Path¶
It can sometimes be useful to see the coefficients for all lambda values or to override default lambda selection. Full regularization path can be extracted from both R and python clients (currently not from Flow). It returns coefficients (and standardized coefficients) for all computed lambda values and also the explained deviances on both train and validation. Subsequently, the makeGLMModel call can be used to create an H2O GLM model with selected coefficients.
To extract the regularization path from R or python:
Solvers¶
This section provides general guidelines for best performance from the GLM implementation details. The optimal solver depends on the data properties and prior information regarding the variables (if available). In general, the data are considered sparse if the ratio of zeros to nonzeros in the input matrix is greater than 10. The solution is sparse when only a subset of the original set of variables is intended to be kept in the model. In a dense solution, all predictors have nonzero coefficients in the final model.
In GLM, you can specify one of the following solvers:
IRLSM: Iteratively Reweighted Least Squares Method (default)
L_BFGS: Limitedmemory BroydenFletcherGoldfarbShanno algorithm
AUTO: Sets the solver based on given data and parameters.
COORDINATE_DESCENT: Coordinate Decent (not available when
family=multinomial
)COORDINATE_DESCENT_NAIVE: Coordinate Decent Naive
GRADIENT_DESCENT_LH: Gradient Descent Likelihood (available for Ordinal family only; default for Ordinal family)
GRADIENT_DESCENT_SQERR: Gradient Descent Squared Error (available for Ordinal family only)
IRLSM and LBFGS¶
IRLSM (the default) uses a Gram Matrix approach, which is efficient for tall and narrow datasets and when running lambda search via a sparse solution. For wider and dense datasets (thousands of predictors and up), the LBFGS solver scales better. If there are fewer than 500 predictors (or so) in the data, then use the default solver (IRLSM). For larger numbers of predictors, we recommend running IRLSM with a lambda search, and then comparing it to LBFGS with just one \(\ell_2\) penalty. For advanced users, we recommend the following general guidelines:
For a dense solution and a dense dataset, use IRLSM if there are fewer than 500 predictors in the data; otherwise, use LBFGS. Set
alpha=0
to include \(\ell_2\) regularization in the elastic net penalty term to avoid inducing sparsity in the model.For a dense solution with a sparse dataset, use IRLSM if there are fewer than 2000 predictors in the data; otherwise, use LBFGS. Set
alpha=0
.For a sparse solution with a dense dataset, use IRLSM with
lambda_search=TRUE
if fewer than 500 active predictors in the solution are expected; otherwise, use LBFGS. Setalpha
to be greater than 0 to add in an \(\ell_1\) penalty to the elastic net regularization, which induces sparsity in the estimated coefficients.For a sparse solution with a sparse dataset, use IRLSM with
lambda_search=TRUE
if you expect less than 5000 active predictors in the solution; otherwise, use LBFGS. Setalpha
to be greater than 0.
If you are unsure whether the solution should be sparse or dense, try both along with a grid of alpha values. The optimal model can be picked based on its performance on the validation data (or alternatively, based on the performance in crossvalidation when not enough data is available to have a separate validation dataset).
Coordinate Descent¶
In addition to IRLSM and LBFGS, H2O’s GLM includes options for specifying Coordinate Descent. Cyclical Coordinate Descent is able to handle large datasets well and deals efficiently with sparse features. It can improve the performance when the data contains categorical variables with a large number of levels, as it is implemented to deal with such variables in a parallelized way.
Coordinate Descent is IRLSM with the covariance updates version of cyclical coordinate descent in the innermost loop. This version is faster when \(N > p\) and \(p\) ~ \(500\).
Coordinate Descent Naive is IRLSM with the naive updates version of cyclical coordinate descent in the innermost loop.
Coordinate Descent provides much better results if lambda search is enabled. Also, with bounds, it tends to get higher accuracy.
Coordinate Descent cannot be used with
family=multinomial
.
Both of the above method are explained in the glmnet paper.
Gradient Descent¶
For Ordinal regression problems, H2O provides options for Gradient Descent. Gradient Descent is a firstorder iterative optimization algorithm for finding the minimum of a function. In H2O’s GLM, conventional ordinal regression uses a likelihood function to adjust the model parameters. The model parameters are adjusted by maximizing the loglikelihood function using gradient descent. When the Ordinal family is specified, the solver
parameter will automatically be set to GRADIENT_DESCENT_LH
. To adjust the model parameters using the loss function, you can set the solver parameter to GRADIENT_DESCENT_SQERR
.
Coefficients Table¶
A Coefficients Table is outputted in a GLM model. This table provides the following information: Column names, Coefficients, Standard Error, zvalue, pvalue, and Standardized Coefficients.
Coefficients are the predictor weights (i.e. the weights used in the actual model used for prediction) in a GLM model.
Standard error, zvalues, and pvalues are classical statistical measures of model quality. pvalues are essentially hypothesis tests on the values of each coefficient. A high pvalue means that a coefficient is unreliable (insiginificant) while a low pvalue suggest that the coefficient is statistically significant.
The standardized coefficients are returned if the
standardize
option is enabled (which is the default). These are the predictor weights of the standardized data and are included only for informational purposes (e.g. to compare relative variable importance). In this case, the “normal” coefficients are obtained from the standardized coefficients by reversing the data standardization process (descaled, with the intercept adjusted by an added offset) so that they can be applied to data in its original form (i.e. no standardization prior to scoring). Note: These are not the same as coefficients of a model built on nonstandardized data.
Extracting Coefficients Table Information¶
You can extract the columns in the Coefficients Table by specifying names
, coefficients
, std_error
, z_value
, p_value
, standardized_coefficients
in a retrieve/print statement. (Refer to the example that follows.) In addition, H2O provides the following builtin methods for retrieving standard and nonstandard coefficients:
coef()
: Coefficients that can be applied to nonstandardized datacoef_norm()
: Coefficients that can be fitted on the standardized data (requiresstandardized=TRUE
, which is the default)
For an example, refer here.
GLM Likelihood¶
Maximum Likelihood Estimation¶
For an initial rough estimate of the parameters \(\hat{\beta}\) you use the estimate to generate fitted values: \(\mu_{i}=g^{1}(\hat{\eta_{i}})\)
Let \(z\) be a working dependent variable such that \(z_{i}=\hat{\eta_{i}}+(y_{i}\hat{\mu_{i}})\frac{d\eta_{i}}{d\mu_{i}}\),
where \(\frac{d\eta_{i}}{d\mu_{i}}\) is the derivative of the link function evaluated at the trial estimate.
Calculate the iterative weights: \(w_{i}=\frac{p_{i}}{[b^{\prime\prime}(\theta_{i})\frac{d\eta_{i}}{d\mu_{i}}^{2}]}\)
where \(b^{\prime\prime}\) is the second derivative of \(b(\theta_{i})\) evaluated at the trial estimate.
Assume \(a_{i}(\phi)\) is of the form \(\frac{\phi}{p_{i}}\). The weight \(w_{i}\) is inversely proportional to the variance of the working dependent variable \(z_{i}\) for current parameter estimates and proportionality factor \(\phi\).
Regress \(z_{i}\) on the predictors \(x_{i}\) using the weights \(w_{i}\) to obtain new estimates of \(\beta\).
\(\hat{\beta}=(\mathbf{X}^{\prime}\mathbf{W}\mathbf{X})^{1}\mathbf{X}^{\prime}\mathbf{W}\mathbf{z}\)
where \(\mathbf{X}\) is the model matrix, \(\mathbf{W}\) is a diagonal matrix of \(w_{i}\), and \(\mathbf{z}\) is a vector of the working response variable \(z_{i}\).
This process is repeated until the estimates \(\hat{\beta}\) change by less than the specified amount.
Likelihood and AIC¶
During model training, simplified formulas of likelihood and AIC are used. After the model is built, the full formula is used to calculate the output of the full log likelihood and full AIC values. The full formula is used to calculate the output of the full log likelihood and full AIC values if the parameter calc_like
is set to True
.
Note
The log likelihood value is not available in the crossvalidation metrics. The AIC value is available and is calculated using the original simplified formula independent of the log likelihood.
The following are the supported GLM families and formulae (the log likelihood is calculated for the i th observation).
Gaussian:
where
\(\phi\) is the dispersion parameter estimation
\(\mu_i\) is the prediction
\(y_i\) is the real value of the target variable
Note
For Gaussian family, you need the dispersion parameter estimate in order to calculate the full log likelihood and AIC. Hence, when calc_like
is set to True
, the parameters compute_p_values
and remove_collinear_columns
are set to True
. The parameter dispersion_parameter_method
is set to "pearson"
by default. However, you can set the dispersion_parameter_method
to deviance
if you prefer.
Binomial:
where
\(\mu_i\) is the probability of 1
\(y_i\) is the real value of the target variable
Quasibinomial:
If the predicted value equals \(y_i\), log likelihood is 0
If \(\mu_i >1\) then \(l(\mu_i (\beta); y_i) = y_i \log \{ \mu_i \}\)
Otherwise, \(l(\mu_i (\beta); y_i) = y_i \log \{ \mu_i \} + (1y_i) \log \{ 1 \mu_i \}\) where
\(\mu_i\) is the probability of 1
\(y_i\) is the real value of the target variable
Fractional Binomial:
where
\(\mu_i\) is the probability of 1
\(y_i\) is the real value of the target variable
Poisson:
where
\(\mu_i\) is the prediction
\(y_i\) is the real value of the target variable
Negative Binomial:
where
\(\mu_i\) is the prediction
\(y_i\) is the real value of the target variable
\(k = \frac{1}{\phi}\) is the dispersion parameter estimation
Note
For Negative Binomial family, you need the dispersion parameter estimate. When the parameter calc_like
is set to True
, the parameters compute_p_values
and remove_collinear_columns
are set to True
for you. By default, the parameter dispersion_parameter_method
is set to "pearson"
. However, you can set dispersion_parameter_method
to "deviance"
or "ml"
if you prefer.
Gamma:
where
\(\mu_i\) is the prediction
\(y_i\) is the real value of the target variable
\(\phi\) is the dispersion parameter estimation
Note
For Gamma family, you need the dispersion parameter estimate. When the parameter calc_like
is set to True
, the parameters compute_p_values
and remove_collinear_columns
are set to True
for you. By default, the parameter dispersion_parameter_method
is set to "pearson"
. However, you can set dispersion_parameter_method
to "deviance"
or "ml"
if you prefer.
Multinomial:
where \(\mu_i\) is the predicted probability of the actual class \(y_i\)
Tweedie:
The Tweedie calculation is located in the section Tweedie Likelihood Calculation.
Note
For Tweedie family, you need the dispersion parameter estimate. When the parameter calc_like
is set to True
, the dispersion_parameter_method
is set to "ml"
which provides you with the best log likelihood estimation.
Final AIC Calculation¶
The final AIC in the output metric is calculated using the standard formula, utilizing the previously computed log likelihood.
where
\(p\) is the number of nonzero coefficients estimated in the model
\(LL\) is the log likelihood
To manage computational intensity, calc_like
is used. This parameter was previously only used for HGLM models, but its utilization has been expanded. By default, calc_like=False
, but you can set it to True
and the parameter HGLM
to False
to enable the calculation of the full log likelihood and full AIC. This computation is performed during the final scoring phase after the model finishes building.
Tweedie Likelihood Calculation¶
There are three different estimations you calculate Tweedie likelihood for:
when you fix the variance power and estimate the dispersion parameter;
when you fix the dispersion parameter and estimate the variance power; or
when you estimate both the variance power and dispersion parameter.
The calculation in this section is used to estimate the full log likelihood. When you fix the Tweedie variance power, you will use a simpler formula (unless you are estimating dispersion). When fixing the Tweedie variance power for dispersion estimation, you use the Series method.
When you fix the variance power and estimate the dispersion parameter, the Series method is used to perform the estimation. In this case, you can actually separate the GLM coefficient estimation and the dispersion parameter estimation at the end of the GLM model building process. Standard Newton’s method is used to estimate the dispersion parameter using the Series method which is an approximation of the Tweedie likelihood function.
Depending on \(p\), \(y\), and \(\phi\), different methods are used for this log likelihood estimation. To start, let:
If \(p=2\), then it will use the log likelihood of the Gamma distribution:
If \(p=3\), then it will use the inverse Gaussian distribution:
If \(p<2\) and \(\xi \leq 0.01\), then it will use the Fourier inversion method.
If \(p>2\) and \(\xi \geq 1\), then it will also use the Fourier inversion method.
Everything else will use the Series method. However, if the Series method fails (output of NaN
), then it will try the Fourier inversion method instead.
If both the Series method and Fourier inversion method fail, or if the Fourier inversion method was chosen based on the \(\xi\) criterium and it failed, it will then estimate the log likelihood using the Saddlepoint approximation.
Here are the general usages for Tweedie variance power and dispersion parameter estimation using maximum likelihood:
fix_tweedie_variance_power = True
andfix_dispersion_parameter = False
as it will use the Tweedie variance power set in parametertweedie_variance_power
and estimate the dispersion parameter starting with the value set in parameterinit_dispersion_parameter
;fix_tweedie_variance_power = False
andfix_dispersion_parameter = True
as it will use the dispersion parameter value in parameterinit_dispersion_parameter
and estimate the Tweedie variance power starting with the value set in parametertweedie_variance_power
;fix_tweedie_variance_power = False
andfix_dispersion_parameter = False
as it will estimate both the variance power and dispersion parameter using the values set intweedie_variance_power
andinit_dispersion_parameter
respectively.
Optimization Procedure
When estimating just the Tweedie variance power, it uses the golden section search. Once a small region is found, then it switches to Newton’s method. If Newton’s method fails (i.e. steps out of the bounds found by the golden section search), it uses the golden section search until convergence. When you optimize both Tweedie variance power and dispersion, it uses the NelderMead method with constraints so that Tweedie variance power \(p>1+10^{10}\) and dispersion \(\phi >10^{10}\). If the NelderMead seems to be stuck in local optimum, you might want to try increasing the dispersion_learning_rate
.
Note
(Applicable for Gamma, Tweedie, and Negative Binomial families) If you set dispersion_parameter_method="ml"
, then solver
must be set to "IRLSM"
.
Variable Inflation Factors¶
The variable inflation factor (VIF) quantifies the inflation of the variable. Variables are inflated due to their correlation with other predictor variables within the model. For each predictor in a multiple regression model, there is a VIF. This process can be calculated with cross validation turned on.
The VIF is constructed by:
setting a numerical predictor x as the response while using the remaining predictors except for y,
building a GLM regression model,
calculating the VIF as \(\frac{1.0}{(1.0R^2)}\) where \(R^2\) is taken from the GLM regression model built in the prior step, and
repeating this process for all remaining numerical predictors to retrieve their VIF.
Variable Inflation Factor Example¶
# Import the training data:
training_data < h2o.importFile("http://h2opublictestdata.s3.amazonaws.com/smalldata/glm_test/gamma_dispersion_factor_9_10kRows.csv")
# Set the predictors and response:
predictors < c('abs.C1.','abs.C2.','abs.C3.','abs.C4.','abs.C5.')
response < 'resp'
# Build and train the model:
vif_glm < h2o.glm(x = predictors,
y = response,
training_frame = training_data,
family = 'gamma',
lambda = 0,
generate_variable_inflation_factors = TRUE,
fold_assignment = 'modulo',
nfolds = 3,
keep_cross_validation_models = TRUE)
# Retrieve the variable inflation factors:
h2o.get_variable_inflation_factors(vif_glm)
abs.C1. abs.C2. abs.C3. abs.C4. abs.C5.
1.000334 1.000173 1.000785 1.000539 1.000535
# Import the GLM estimator:
from h2o.estimators import H2OGeneralizedLinearEstimator
# Import the training data:
training_data = h2o.import_file("http://h2opublictestdata.s3.amazonaws.com/smalldata/glm_test/gamma_dispersion_factor_9_10kRows.csv")
# Set the predictors and response:
predictors = ["abs.C1.","abs.C2.","abs.C3.","abs.C4.","abs.C5.""]
response = "resp"
# Build and train the model:
vif_glm = H2OGeneralizedLinearEstimator(family="gamma",
lambda_=0,
generate_variable_inflation_factors=True,
fold_assignment="modulo",
nfolds=3,
keep_cross_validation_models=True)
vif_glm.train(x=predictors, y=response, training_frame=training_data)
# Retrieve the variable inflation factors:
vif_glm.get_variable_inflation_factors()
{'Intercept': nan, 'abs.C1.': 1.0003341467438167, 'abs.C2.': 1.0001734204183244, 'abs.C3.': 1.0007846189027745, 'abs.C4.': 1.0005388379729434, 'abs.C5.': 1.0005349427184604}
Modifying or Creating a Custom GLM Model¶
In R and Python, the makeGLMModel
call can be used to create an H2O model from given coefficients. It needs a source GLM model trained on the same dataset to extract the dataset information. To make a custom GLM model from R or Python:
R: call
h2o.makeGLMModel
. This takes a model, a vector of coefficients, and (optional) decision threshold as parameters.Python:
H2OGeneralizedLinearEstimator.makeGLMModel
(static method) takes a model, a dictionary containing coefficients, and (optional) decision threshold as parameters.
Examples¶
Below is a simple example showing how to build a Generalized Linear model.
library(h2o)
h2o.init()
df < h2o.importFile("https://h2opublictestdata.s3.amazonaws.com/smalldata/prostate/prostate.csv")
df$CAPSULE < as.factor(df$CAPSULE)
df$RACE < as.factor(df$RACE)
df$DCAPS < as.factor(df$DCAPS)
df$DPROS < as.factor(df$DPROS)
predictors < c("AGE", "RACE", "VOL", "GLEASON")
response < "CAPSULE"
prostate_glm < h2o.glm(family = "binomial",
x = predictors,
y = response,
training_frame = df,
lambda = 0,
compute_p_values = TRUE
generate_scoring_history = TRUE)
# Coefficients that can be applied to the nonstandardized data
h2o.coef(prostate_glm)
Intercept RACE.1 RACE.2 AGE VOL GLEASON
6.67515539 0.44278752 0.58992326 0.01788870 0.01278335 1.25035939
# Coefficients fitted on the standardized data (requires standardize=TRUE, which is on by default)
h2o.coef_norm(prostate_glm)
Intercept RACE.1 RACE.2 AGE VOL GLEASON
0.07610006 0.44278752 0.58992326 0.11676080 0.23454402 1.36533415
# Print the coefficients table
prostate_glm@model$coefficients_table
Coefficients: glm coefficients
names coefficients std_error z_value p_value standardized_coefficients
1 Intercept 6.675155 1.931760 3.455478 0.000549 0.076100
2 RACE.1 0.442788 1.324231 0.334373 0.738098 0.442788
3 RACE.2 0.589923 1.373466 0.429514 0.667549 0.589923
4 AGE 0.017889 0.018702 0.956516 0.338812 0.116761
5 VOL 0.012783 0.007514 1.701191 0.088907 0.234544
6 GLEASON 1.250359 0.156156 8.007103 0.000000 1.365334
# Print the standard error
prostate_glm@model$coefficients_table$std_error
[1] 1.931760363 1.324230832 1.373465793 0.018701933 0.007514354 0.156156271
# Print the p values
prostate_glm@model$coefficients_table$p_value
[1] 5.493181e04 7.380978e01 6.675490e01 3.388116e01 8.890718e02
[6] 1.221245e15
# Print the z values
prostate_glm@model$coefficients_table$z_value
[1] 3.4554780 0.3343734 0.4295143 0.9565159 1.7011907 8.0071033
# Retrieve a graphical plot of the standardized coefficient magnitudes
h2o.std_coef_plot(prostate_glm)
# Since you generated the scoring history, you can retrieve the average objective and the negative log likelihood:
print(h2o.average_objective(prostate_glm))
[1] 0.540688
print(h2o.negative_log_likelihood(prostate_glm))
[1] 205.4614
import h2o
h2o.init()
from h2o.estimators.glm import H2OGeneralizedLinearEstimator
prostate = h2o.import_file("https://h2opublictestdata.s3.amazonaws.com/smalldata/prostate/prostate.csv")
prostate['CAPSULE'] = prostate['CAPSULE'].asfactor()
prostate['RACE'] = prostate['RACE'].asfactor()
prostate['DCAPS'] = prostate['DCAPS'].asfactor()
prostate['DPROS'] = prostate['DPROS'].asfactor()
predictors = ["AGE", "RACE", "VOL", "GLEASON"]
response_col = "CAPSULE"
prostate_glm = H2OGeneralizedLinearEstimator(family= "binomial",
lambda_ = 0,
compute_p_values = True
generate_scoring_history = True)
prostate_glm.train(predictors, response_col, training_frame= prostate)
# Coefficients that can be applied to the nonstandardized data.
print(prostate_glm.coef())
{u'GLEASON': 1.2503593867263176, u'VOL': 0.012783348665664449, u'AGE': 0.017888697161812357, u'Intercept': 6.6751553940827195, u'RACE.2': 0.5899232636956354, u'RACE.1': 0.44278751680880707}
# Coefficients fitted on the standardized data (requires standardize = True, which is on by default)
print(prostate_glm.coef_norm())
{u'GLEASON': 1.365334151581163, u'VOL': 0.2345440232267344, u'AGE': 0.11676080128780757, u'Intercept': 0.07610006436753876, u'RACE.2': 0.5899232636956354, u'RACE.1': 0.44278751680880707}
# Print the Coefficients table
prostate_glm._model_json['output']['coefficients_table']
Coefficients: glm coefficients
names coefficients std_error z_value p_value standardized_coefficients
     
Intercept 6.67516 1.93176 3.45548 0.000549318 0.0761001
RACE.1 0.442788 1.32423 0.334373 0.738098 0.442788
RACE.2 0.589923 1.37347 0.429514 0.667549 0.589923
AGE 0.0178887 0.0187019 0.956516 0.338812 0.116761
VOL 0.0127833 0.00751435 1.70119 0.0889072 0.234544
GLEASON 1.25036 0.156156 8.0071 1.22125e15 1.36533
# Print the Standard error
print(prostate_glm._model_json['output']['coefficients_table']['std_error'])
[1.9317603626604352, 1.3242308316851008, 1.3734657932878116, 0.01870193337051072, 0.007514353657915356, 0.15615627100850296]
# Print the p values
print(prostate_glm._model_json['output']['coefficients_table']['p_value'])
[0.0005493180609459358, 0.73809783692024, 0.6675489550762566, 0.33881164088847204, 0.0889071809658667, 1.2212453270876722e15]
# Print the z values
print(prostate_glm._model_json['output']['coefficients_table']['z_value'])
[3.4554779791058787, 0.3343733631736653, 0.42951434726559384, 0.9565159284557886, 1.7011907141473064, 8.007103260414265]
# Retrieve a graphical plot of the standardized coefficient magnitudes
prostate_glm.std_coef_plot()
# Since you generated the scoring history, you can access the average objective and negative log likelihood:
print("average objective: {0}.".format(prostate_glm.average_objective()))
average objective: 0.5406879877388551.
print("negative log likelihood: {0}.".format(prostate_glm.negative_log_likelihood()))
negative log likelihood: 205.46143534076492.
Calling Model Attributes¶
While not all model attributes have their own callable APIs, you can still retrieve their information. Using the previous example, here is how to call a model’s attributes:
# Retrieve all model attributes:
prostate_glm@model$model_summary
GLM Model: summary
family link regularization number_of_predictors_total
1 binomial logit None 5
number_of_active_predictors number_of_iterations training_frame
1 5 4 RTMP_sid_8b2d_6
# Retrieve a specific model attribute (for example, the number of active predictors):
prostate_glm@model$model_summary['number_of_active_predictors']
number_of_active_predictors
1 5
# Retrieve all model attributes:
prostate_glm._model_json["output"]['model_summary']
GLM Model: summary
family link regularization number_of_predictors_total number_of_active_predictors number_of_iterations training_frame
       
binomial logit None 5 5 4 py_4_sid_9981
# Retrieve a specific model attribute (for example, the number of active predictors):
prostate_glm._model_json["output"]['model_summary']['number_of_active_predictors']
['5']
FAQ¶
How does the algorithm handle missing values during training?
Depending on the selected missing value handling policy, they are either imputed mean or the whole row is skipped. The default behavior is Mean Imputation. Note that unseen categorical levels are replaced by the most frequent level present in training (mod). Optionally, GLM can skip all rows with any missing values.
How does the algorithm handle missing values during testing?
Same as during training. If the missing value handling is set to Skip and we are generating predictions, skipped rows will have Na (missing) prediction.
What happens if the response has missing values?
The rows with missing responses are ignored during model training and validation.
What happens during prediction if the new sample has categorical levels not seen in training?
The value will be filled with either 0 or replaced by the most frequent level present in training (if
missing_value_handling
was set to MeanImputation).
How are unseen categorical values treated during scoring?
Unseen categorical levels are treated based on the missing values handling during training. If your missing value handling was set to Mean Imputation, the unseen levels are replaced by the most frequent level present in training (mod). If your missing value treatment was Skip, the variable is ignored for the given observation.
Does it matter if the data is sorted?
No.
Should data be shuffled before training?
No.
How does the algorithm handle highly imbalanced data in a response column?
GLM does not require special handling for imbalanced data.
What if there are a large number of columns?
IRLS will get quadratically slower with the number of columns. Try LBFGS for datasets with more than 510 thousand columns.
What if there are a large number of categorical factor levels?
GLM internally onehot encodes the categorical factor levels; the same limitations as with a high column count will apply.
When building the model, does GLM use all features or a selection of the best features?
Typically, GLM picks the best predictors, especially if lasso is used (
alpha = 1
). By default, the GLM model includes an L1 penalty and will pick only the most predictive predictors.
When running GLM, is it better to create a cluster that uses many smaller nodes or fewer larger nodes?
A rough heuristic would be:
\(nodes ~=M *N^2/(p * 1e8)\)
where \(M\) is the number of observations, \(N\) is the number of columns (categorical columns count as a single column in this case), and \(p\) is the number of CPU cores per node.
For example, a dataset with 250 columns and 1M rows would optimally use about 20 nodes with 32 cores each (following the formula \(250^2 *1000000/(32* 1e8) = 19.5 ~= 20)\).
How is variable importance calculated for GLM?
For GLM, the variable importance represents the coefficient magnitudes.
How does GLM define and check for convergence during logistic regression?
GLM includes three convergence criteria outside of max iterations:
beta_epsilon
: beta stops changing. This is used mostly with IRLSM.
gradient_epsilon
: gradient is too small. This is used mostly with LBFGS.
objective_epsilon
: relative objective improvement is too small. This is used by all solvers.The default values below are based on a heuristic:
The default for
beta_epsilon
is 1e4.The default for
gradient_epsilon
is 1e6 if there is no regularization (lambda = 0
) or you are running withlambda_search
; 1e4 otherwise.The default for
objective_epsilon
is 1e6 iflambda = 0
; 1e4 otherwise.The default for
max_iterations
depends on the solver type and whether you run with lambda search:
for IRLSM, the default is 50 if no lambda search; 10* number of lambdas otherwise
for LBFGS, the default is number of classes (1 if not classification) * max(20, number of predictors /4 ) if no lambda search; it is number of classes * 100 * nlambdas with lambda search.
You will receive a warning if you reach the maximum number of iterations. In some cases, GLM can end prematurely if it can not progress forward via line search. This typically happens when running a lambda search with IRLSM solver. Note that using CoordinateDescent solver fixes the issue.
Why do I receive different results when I run R’s glm and H2O’s glm?
H2O’s glm and R’s glm do not run the same way and, thus, will provide different results. This is mainly due to the fact that H2O’s glm uses H2O math, H2O objects, and H2O distributed computing. Additionally, H2O’s glm by default adds regularization, so it is essentially solving a different problem.
How can I get H2O’s GLM to match R’s `glm()` function?
There are a few arguments you need to set in order to get H2O’s GLM to match R’s GLM because by default, they do not function the same way. To match R’s GLM, you must set the following in H2O’s GLM:
solver = "IRLSM" lambda = 0 remove_collinear_columns = TRUE compute_p_values = TRUENote:
beta_constraints
must not be set.
GLM Algorithm¶
Following the definitive text by P. McCullagh and J.A. Nelder (1989) on the generalization of linear models to nonlinear distributions of the response variable Y, H2O fits GLM models based on the maximum likelihood estimation via iteratively reweighed least squares.
Let \(y_{1},…,y_{n}\) be n observations of the independent, random response variable \(Y_{i}\).
Assume that the observations are distributed according to a function from the exponential family and have a probability density function of the form:
\(f(y_{i})=exp[\frac{y_{i}\theta_{i}  b(\theta_{i})}{a_{i}(\phi)} + c(y_{i}; \phi)]\) where \(\theta\) and \(\phi\) are location and scale parameters, and \(a_{i}(\phi)\), \(b_{i}(\theta{i})\), and \(c_{i}(y_{i}; \phi)\) are known functions.
\(a_{i}\) is of the form \(a_{i}= \frac{\phi}{p_{i}}\) where \(p_{i}\) is a known prior weight.
When \(Y\) has a pdf from the exponential family:
\(E(Y_{i})=\mu_{i}=b^{\prime} var(Y_{i})=\sigma_{i}^2=b^{\prime\prime}(\theta_{i})a_{i}(\phi)\)
Let \(g(\mu_{i})=\eta_{i}\) be a monotonic, differentiable transformation of the expected value of \(y_{i}\). The function \(\eta_{i}\) is the link function and follows a linear model.
\(g(\mu_{i})=\eta_{i}=\mathbf{x_{i}^{\prime}}\beta\)
When inverted: \(\mu=g^{1}(\mathbf{x_{i}^{\prime}}\beta)\)
Cost of computation¶
H2O can process large data sets because it relies on parallel processes. Large data sets are divided into smaller data sets and processed simultaneously and the results are communicated between computers as needed throughout the process.
In GLM, data are split by rows but not by columns, because the predicted Y values depend on information in each of the predictor variable vectors. If O is a complexity function, N is the number of observations (or rows), and P is the number of predictors (or columns) then
\(Runtime \propto p^3+\frac{(N*p^2)}{CPUs}\)
Distribution reduces the time it takes an algorithm to process because it decreases N.
Relative to P, the larger that (N/CPUs) becomes, the more trivial p becomes to the overall computational cost. However, when p is greater than (N/CPUs), O is dominated by p.
\(Complexity = O(p^3 + N*p^2)\)
References¶
Breslow, N E. “Generalized Linear Models: Checking Assumptions and Strengthening Conclusions.” Statistica Applicata 8 (1996): 2341.
Peter K. Dunn, Gordon K. Symth, “Series evaluation of Tweedie exponential dispersion model densities”, Statistics and Computing, Volume 15 (2005), pages 267280.
Frome, E L. “The Analysis of Rates Using Poisson Regression Models.” Biometrics (1983): 665674.
Lee, Y and Nelder, J. A. Hierarchical generalized linear models with discussion. J. R. Statist.Soc. B, 58:619678, 1996.
Lee, Y and Nelder, J. A. and Y. Pawitan. Generalized linear models with random effects. Chapman & Hall/CRC, 2006.
Snee, Ronald D. “Validation of Regression Models: Methods and Examples.” Technometrics 19.4 (1977): 415428.