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We've seen two extremes: squared loss optimizes efficiency when data is clean, targeting the conditional mean with smooth, well-behaved gradients. Absolute loss prioritizes robustness, ignoring outlier magnitude to target the conditional median. Each has clear strengths—and equally clear weaknesses.
But must we choose? What if we could have the statistical efficiency of squared loss for normal observations while maintaining the robustness of absolute loss for outliers?
Enter the Huber loss, proposed by Peter Huber in 1964 as part of his foundational work on robust statistics. This elegant hybrid acts like squared loss when errors are small and like absolute loss when errors are large. The transition between these regimes is controlled by a single parameter $\delta$, giving us a tunable balance between efficiency and robustness.
The Huber loss is one of the most successful examples of robust estimation—a field that asks: how can we design estimators that work well even when our assumptions about the data are violated?
By the end of this page, you will understand the Huber loss function in depth—its piecewise definition, the role of the δ parameter, gradient and Hessian computation, connection to M-estimation, and implementation in gradient boosting. You'll learn how to choose δ and when Huber loss outperforms both squared and absolute losses.
The Huber loss function is defined piecewise:
$$L_\delta(y, \hat{y}) = \begin{cases} \frac{1}{2}(y - \hat{y})^2 & \text{if } |y - \hat{y}| \leq \delta \ \delta|y - \hat{y}| - \frac{1}{2}\delta^2 & \text{if } |y - \hat{y}| > \delta \end{cases}$$
Alternatively, using the residual $r = y - \hat{y}$:
$$L_\delta(r) = \begin{cases} \frac{1}{2}r^2 & \text{if } |r| \leq \delta \ \delta|r| - \frac{1}{2}\delta^2 & \text{if } |r| > \delta \end{cases}$$
The Parameter δ (Delta):
At r = δ, the quadratic piece gives L = δ²/2. For continuity, the linear piece (δ·|r| - C) must also equal δ²/2 when |r| = δ. Solving: δ·δ - C = δ²/2, so C = δ²/2. This ensures the loss function and its derivative are continuous at the transition point.
Understanding the Shape:
The Huber loss can be visualized as:
Unlike absolute loss (V-shaped with a corner), Huber is smooth everywhere—the derivative exists at all points including $r = \pm\delta$. This smoothness enables standard gradient-based optimization.
Limiting Cases:
Thus, $\delta$ interpolates between squared and absolute loss, with extreme values recovering the pure forms.
| Residual (r) | Huber Loss | Squared Loss | Absolute Loss |
|---|---|---|---|
| 0 | 0 | 0 | 0 |
| ±0.5 | 0.125 | 0.125 | 0.5 |
| ±1 (= δ) | 0.5 | 0.5 | 1 |
| ±2 | 1.5 | 2 | 2 |
| ±5 | 4.5 | 12.5 | 5 |
| ±10 | 9.5 | 50 | 10 |
| ±100 | 99.5 | 5000 | 100 |
Observations from the Table:
The gradient and Hessian of Huber loss are what make it computationally tractable and well-suited for gradient boosting.
Computing the Gradient:
For $|r| \leq \delta$ (quadratic region): $$\frac{\partial L}{\partial \hat{y}} = -(y - \hat{y}) = \hat{y} - y$$
For $|r| > \delta$ (linear region): $$\frac{\partial L}{\partial \hat{y}} = -\delta \cdot \text{sign}(y - \hat{y}) = \delta \cdot \text{sign}(\hat{y} - y)$$
Unified Form:
$$g = \frac{\partial L}{\partial \hat{y}} = \begin{cases} \hat{y} - y & \text{if } |y - \hat{y}| \leq \delta \ \delta \cdot \text{sign}(\hat{y} - y) & \text{if } |y - \hat{y}| > \delta \end{cases}$$
Or equivalently, the gradient is the residual clipped to $[-\delta, \delta]$: $$g = \text{clip}(\hat{y} - y, -\delta, \delta)$$
The Huber gradient is simply the squared loss gradient (the residual) clipped to ±δ. Large errors don't produce gradients larger than δ in magnitude. This clipping is what provides robustness—outliers can't dominate the gradient signal with arbitrarily large values.
Computing the Hessian:
The Hessian (second derivative) is:
For $|r| \leq \delta$: $$h = \frac{\partial^2 L}{\partial \hat{y}^2} = 1$$
For $|r| > \delta$: $$h = \frac{\partial^2 L}{\partial \hat{y}^2} = 0$$
Unified Form: $$h = \mathbf{1}_{|r| \leq \delta} = \begin{cases} 1 & \text{if } |y - \hat{y}| \leq \delta \ 0 & \text{if } |y - \hat{y}| > \delta \end{cases}$$
Interpretation:
XGBoost-Style Optimization:
In XGBoost, new trees are found by optimizing: $$\sum_i \left[ g_i f(x_i) + \frac{1}{2} h_i f(x_i)^2 \right] + \Omega(f)$$
For points with $h_i = 0$ (outliers), the quadratic term vanishes—only the linear gradient term remains. This naturally downweights outliers in tree construction.
| Residual (r) | Huber Gradient | Squared Gradient | Huber Hessian | Squared Hessian |
|---|---|---|---|---|
| 0 | 0 | 0 | 1 | 1 |
| +0.5 | +0.5 | +0.5 | 1 | 1 |
| +1 (= δ) | +1 | +1 | 1 | 1 |
| +2 | +1 (clipped) | +2 | 0 | 1 |
| +10 | +1 (clipped) | +10 | 0 | 1 |
| +100 | +1 (clipped) | +100 | 0 | 1 |
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import numpy as np class HuberLoss: """ Huber loss implementation for gradient boosting. Combines squared loss (small errors) with absolute loss (large errors). """ def __init__(self, delta=1.0): """ Args: delta: Threshold between quadratic and linear regions. - Small delta: More robust, closer to absolute loss - Large delta: More efficient, closer to squared loss """ self.delta = delta def loss(self, y_true, y_pred): """Compute Huber loss.""" residual = y_true - y_pred abs_residual = np.abs(residual) # Quadratic region: |r| <= delta quadratic_mask = abs_residual <= self.delta quadratic_loss = 0.5 * residual**2 # Linear region: |r| > delta linear_loss = self.delta * abs_residual - 0.5 * self.delta**2 return np.where(quadratic_mask, quadratic_loss, linear_loss) def gradient(self, y_true, y_pred): """ Compute gradient: clipped residual. This is the negative of the pseudo-residual used in gradient boosting. """ residual = y_pred - y_true # Note: pred - true, not true - pred return np.clip(residual, -self.delta, self.delta) def negative_gradient(self, y_true, y_pred): """ Compute negative gradient (pseudo-residual for gradient boosting). This is what trees are trained to predict. """ return -self.gradient(y_true, y_pred) def hessian(self, y_true, y_pred): """ Compute Hessian: 1 for small residuals, 0 for large. Used in XGBoost-style second-order methods. """ residual = y_true - y_pred return (np.abs(residual) <= self.delta).astype(float) def visualize_huber_vs_alternatives(): """Visualize Huber loss compared to squared and absolute loss.""" import matplotlib.pyplot as plt residuals = np.linspace(-5, 5, 1000) delta = 1.5 # Compute losses huber = HuberLoss(delta=delta) huber_loss = huber.loss(residuals, 0) # y_true=r, y_pred=0 squared_loss = 0.5 * residuals**2 absolute_loss = np.abs(residuals) # Plot fig, axes = plt.subplots(1, 2, figsize=(14, 5)) # Loss curves axes[0].plot(residuals, squared_loss, label='Squared Loss', linewidth=2) axes[0].plot(residuals, absolute_loss, label='Absolute Loss', linewidth=2) axes[0].plot(residuals, huber_loss, label=f'Huber Loss (δ={delta})', linewidth=2, linestyle='--') axes[0].axvline(x=delta, color='gray', linestyle=':', alpha=0.5) axes[0].axvline(x=-delta, color='gray', linestyle=':', alpha=0.5) axes[0].set_xlabel('Residual') axes[0].set_ylabel('Loss') axes[0].set_title('Loss Functions Comparison') axes[0].legend() axes[0].set_ylim(0, 12) axes[0].grid(True, alpha=0.3) # Gradient curves huber_grad = huber.gradient(residuals, 0) squared_grad = residuals absolute_grad = np.sign(residuals) axes[1].plot(residuals, squared_grad, label='Squared Loss', linewidth=2) axes[1].plot(residuals, absolute_grad, label='Absolute Loss', linewidth=2) axes[1].plot(residuals, huber_grad, label=f'Huber Loss (δ={delta})', linewidth=2, linestyle='--') axes[1].axvline(x=delta, color='gray', linestyle=':', alpha=0.5) axes[1].axvline(x=-delta, color='gray', linestyle=':', alpha=0.5) axes[1].set_xlabel('Residual') axes[1].set_ylabel('Gradient') axes[1].set_title('Gradient Functions Comparison') axes[1].legend() axes[1].grid(True, alpha=0.3) plt.tight_layout() plt.savefig('huber_comparison.png', dpi=150) print("Saved visualization to huber_comparison.png") # Example usageif __name__ == "__main__": # Demonstrate gradient clipping huber = HuberLoss(delta=1.0) residuals = np.array([0.0, 0.5, 1.0, 2.0, 5.0, 10.0, 100.0]) print("Huber Loss Gradient Analysis (δ = 1.0)") print("=" * 60) print(f"{'Residual':>10} {'Huber Grad':>12} {'Squared Grad':>14} {'Hessian':>10}") print("-" * 60) for r in residuals: hg = huber.gradient(np.array([r]), np.array([0]))[0] sg = r h = huber.hessian(np.array([r]), np.array([0]))[0] print(f"{r:>10.1f} {hg:>12.1f} {sg:>14.1f} {h:>10.0f}") print() print("Notice: Huber gradient is clipped to [-1, 1]") print("Notice: Hessian is 0 for |residual| > δ")The delta parameter is crucial—it defines what counts as an "outlier." Choosing it well is essential for good performance.
Intuition for δ:
Common Approaches:
1. Fixed Value (Default):
Many implementations default to $\delta = 1.0$ or $\delta = 1.35$. The value 1.35 is chosen because, for standard normal data, Huber loss with $\delta = 1.35$ achieves 95% of the efficiency of the mean while being much more robust.
2. Scale-Based:
Set $\delta$ based on the scale of residuals: $$\delta = k \cdot \text{MAD}$$
Where MAD = Median Absolute Deviation of residuals, and $k$ is typically 1-3. This automatically adapts to the data scale.
3. Cross-Validation:
Treat $\delta$ as a hyperparameter and tune it via cross-validation. This is most principled but computationally expensive.
4. Percentile-Based:
Set $\delta$ to the $p$-th percentile of absolute residuals (e.g., 90th percentile). This treats the top 10% of errors as outliers.
Peter Huber showed that δ ≈ 1.345σ (where σ is the standard deviation) gives 95% asymptotic efficiency relative to the mean for Gaussian data. This is often approximated as MAD × 1.345/0.6745 ≈ MAD × 2, where MAD is the median absolute deviation from the median.
| δ Value | Behavior | When to Use |
|---|---|---|
| Very small (0.1) | Almost like absolute loss | Extreme outlier contamination |
| Small (0.5-1) | Robust with some efficiency | Moderate contamination expected |
| Medium (1-2) | Balanced efficiency/robustness | Light contamination, general use |
| Large (5+) | Almost like squared loss | Clean data, few outliers |
| Adaptive | Based on data | Best general approach |
Dynamic δ in Gradient Boosting:
Some implementations allow δ to change during training:
Start large, decrease: Begin with squared-loss-like behavior for fast initial learning, then decrease δ to robustify as residuals shrink.
Residual-adaptive: Compute δ based on current residual distribution (e.g., 90th percentile). As the model improves, δ automatically adjusts.
Fixed throughout: Simple and reproducible. Most common in practice.
Best Practice:
Start with $\delta = 1.0$ or use the MAD-based estimate. If performance is unsatisfactory, tune via cross-validation or try the percentile approach.
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import numpy as npfrom scipy.stats import median_abs_deviation def estimate_huber_delta(residuals, method='mad', percentile=90): """ Estimate optimal delta for Huber loss. Args: residuals: Array of prediction residuals method: 'mad', 'percentile', or 'iqr' percentile: Used when method='percentile' Returns: Estimated delta value """ abs_residuals = np.abs(residuals) if method == 'mad': # Median Absolute Deviation based # For Gaussian: MAD ≈ 0.6745 * σ # Huber optimal δ ≈ 1.345 * σ # So δ ≈ MAD * 1.345 / 0.6745 ≈ MAD * 2 mad = median_abs_deviation(residuals) return mad * 2.0 # Approximate 95% efficiency elif method == 'percentile': # Treat top (100-percentile)% as outliers return np.percentile(abs_residuals, percentile) elif method == 'iqr': # Interquartile range based q75, q25 = np.percentile(abs_residuals, [75, 25]) iqr = q75 - q25 return 1.5 * iqr # Common outlier threshold else: raise ValueError(f"Unknown method: {method}") def tune_delta_cv(X, y, delta_range, n_folds=5): """ Tune delta via cross-validation. This is the most principled approach but computationally expensive. """ from sklearn.model_selection import cross_val_score from sklearn.ensemble import GradientBoostingRegressor results = {} for delta in delta_range: # Note: sklearn uses 'alpha' parameter for Huber loss model = GradientBoostingRegressor( loss='huber', alpha=0.9, # This controls delta indirectly n_estimators=100, random_state=42 ) # Cross-validation with MAE scoring (robust metric) scores = cross_val_score(model, X, y, scoring='neg_mean_absolute_error', cv=n_folds) results[delta] = -scores.mean() best_delta = min(results, key=results.get) return best_delta, results # Demonstrationif __name__ == "__main__": # Generate data with outliers np.random.seed(42) n = 1000 # Normal residuals residuals = np.random.normal(0, 1, n) # Add 5% outliers outlier_idx = np.random.choice(n, int(0.05 * n), replace=False) residuals[outlier_idx] += np.random.choice([-1, 1], len(outlier_idx)) * 10 print("Delta Selection Methods") print("=" * 50) for method in ['mad', 'percentile', 'iqr']: delta = estimate_huber_delta(residuals, method=method) print(f"{method:12s}: δ = {delta:.4f}") print() print(f"Residual std (contaminated): {np.std(residuals):.4f}") print(f"Residual std (robust, MAD×1.5): {median_abs_deviation(residuals) * 1.4826:.4f}")Huber loss is a special case of M-estimation, a general framework for robust parameter estimation introduced by Peter Huber in 1964.
What is M-Estimation?
M-estimation minimizes a sum of functions of residuals:
$$\hat{\theta} = \arg\min_\theta \sum_{i=1}^{n} \rho(y_i - f(x_i; \theta))$$
Where $\rho$ is called the objective function or loss function. Different choices of $\rho$ give different estimators:
The Influence Function and ψ:
The derivative $\psi(r) = \rho'(r)$ is called the influence function or score function. It determines how sensitive the estimator is to observations:
Huber recognized that bounded influence functions provide robustness, but pure absolute loss sacrifices too much efficiency. His genius was finding the balance: be efficient (quadratic) where it helps, be robust (linear) where it matters. The Huber loss is optimal in this tradeoff under certain contamination models.
The Contamination Model:
Huber analyzed the ε-contamination model: data comes from a mixture:
$$(1-\epsilon) \cdot \mathcal{N}(\mu, \sigma^2) + \epsilon \cdot H$$
Where:
Minimax Optimality:
Huber proved that for this contamination model, the Huber loss is minimax optimal: it minimizes the maximum possible variance across all contaminating distributions $H$.
This is why Huber loss is so widely used—it's not just intuitive, it's theoretically optimal for the contamination scenario we often face in practice.
Connection to Gradient Boosting:
In gradient boosting, each tree fits the ψ (influence) function evaluated at current residuals:
$$h_m \text{ fits } {(x_i, \psi(r_i)) : i = 1, \ldots, n}$$
For Huber loss, this means fitting clipped residuals. Points with $|r_i| > \delta$ contribute only their direction (capped at $\pm\delta$), not their full magnitude.
Let's walk through how Huber loss integrates into the gradient boosting algorithm.
Algorithm Steps:
Initialize: $F_0(x) = \arg\min_c \sum_i L_\delta(y_i, c)$
For Huber loss, the optimal constant minimizes a mix of squared and absolute deviations. When most residuals are within δ, this is close to the mean; otherwise, it's closer to the median.
For each iteration m:
a. Compute residuals: $r_i = y_i - F_{m-1}(x_i)$
b. Compute pseudo-residuals (clipped): $\tilde{r}_i = \text{clip}(r_i, -\delta, \delta)$
c. Fit tree $h_m$ to pseudo-residuals $(x_i, \tilde{r}_i)$
d. For each leaf $j$, compute optimal value: $$w_j = \arg\min_w \sum_{i \in I_j} L_\delta(y_i, F_{m-1}(x_i) + w)$$
e. Update: $F_m(x) = F_{m-1}(x) + \eta \cdot h_m(x)$
The Leaf Value Problem:
Step (d) is more complex for Huber than for squared loss. There's no closed-form solution. Implementations use:
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import numpy as npfrom sklearn.tree import DecisionTreeRegressor class HuberGradientBoosting: """ Gradient Boosting with Huber Loss. Key differences from squared loss: 1. Pseudo-residuals are clipped to [-delta, delta] 2. Leaf values require optimization (not just mean) 3. Robust to outliers while maintaining efficiency """ def __init__(self, n_estimators=100, learning_rate=0.1, max_depth=3, delta=1.0): self.n_estimators = n_estimators self.learning_rate = learning_rate self.max_depth = max_depth self.delta = delta self.trees = [] self.initial_prediction = None def _huber_loss(self, y_true, y_pred): """Compute mean Huber loss.""" residual = y_true - y_pred abs_residual = np.abs(residual) quadratic = 0.5 * residual**2 linear = self.delta * abs_residual - 0.5 * self.delta**2 loss = np.where(abs_residual <= self.delta, quadratic, linear) return np.mean(loss) def _pseudo_residuals(self, y_true, y_pred): """ Compute pseudo-residuals (negative gradient). For Huber: clip residuals to [-delta, delta] """ residuals = y_true - y_pred return np.clip(residuals, -self.delta, self.delta) def _compute_leaf_value(self, residuals): """ Find optimal leaf value for Huber loss. Uses weighted median approximation for efficiency. For exact solution, use numerical optimization. """ # Approximate: use median of residuals # (exact for pure absolute loss, good approximation for Huber) return np.median(residuals) def _compute_leaf_values(self, tree, X, y, current_pred): """Compute optimal values for each leaf.""" leaf_indices = tree.apply(X) residuals = y - current_pred unique_leaves = np.unique(leaf_indices) leaf_values = {} for leaf in unique_leaves: mask = leaf_indices == leaf leaf_residuals = residuals[mask] leaf_values[leaf] = self._compute_leaf_value(leaf_residuals) return leaf_values, leaf_indices def fit(self, X, y): """Fit gradient boosting ensemble with Huber loss.""" n_samples = len(y) # Initialize with median (robust initial estimate) self.initial_prediction = np.median(y) # Current predictions F = np.full(n_samples, self.initial_prediction) print(f"Gradient Boosting with Huber Loss (δ = {self.delta})") print("=" * 60) print(f"Initial prediction: {self.initial_prediction:.4f}") print(f"Initial loss: {self._huber_loss(y, F):.4f}") print() for m in range(self.n_estimators): # Compute pseudo-residuals (clipped) pseudo_residuals = self._pseudo_residuals(y, F) # Fit tree to pseudo-residuals tree = DecisionTreeRegressor(max_depth=self.max_depth) tree.fit(X, pseudo_residuals) # Compute optimal leaf values leaf_values, leaf_indices = self._compute_leaf_values( tree, X, y, F ) # Get predictions using leaf values predictions = np.array([leaf_values[leaf] for leaf in leaf_indices]) # Update ensemble F += self.learning_rate * predictions # Store tree and leaf values self.trees.append((tree, leaf_values)) # Progress tracking if (m + 1) % 20 == 0 or m == 0: loss = self._huber_loss(y, F) print(f"Iteration {m+1:3d}: Huber Loss = {loss:.6f}") print(f"\nFinal Huber Loss: {self._huber_loss(y, F):.6f}") return self def predict(self, X): """Generate predictions.""" predictions = np.full(len(X), self.initial_prediction) for tree, leaf_values in self.trees: leaf_indices = tree.apply(X) tree_preds = np.array([leaf_values.get(l, 0) for l in leaf_indices]) predictions += self.learning_rate * tree_preds return predictions # Compare all three loss functionsif __name__ == "__main__": from sklearn.datasets import make_regression from sklearn.model_selection import train_test_split from sklearn.ensemble import GradientBoostingRegressor # Generate data with outliers X, y = make_regression(n_samples=1000, n_features=10, noise=5, random_state=42) # Add outliers outlier_idx = np.random.choice(len(y), 50, replace=False) y[outlier_idx] += np.random.choice([-1, 1], 50) * 100 X_train, X_test, y_train, y_test = train_test_split(X, y, test_size=0.2) print("\nComparison: Squared vs Huber vs Absolute Loss") print("=" * 60) losses = ['squared_error', 'huber', 'absolute_error'] for loss in losses: model = GradientBoostingRegressor( loss=loss, n_estimators=100, learning_rate=0.1, random_state=42 ) model.fit(X_train, y_train) y_pred = model.predict(X_test) mse = np.mean((y_test - y_pred) ** 2) mae = np.mean(np.abs(y_test - y_pred)) print(f"{loss:15s}: MSE = {mse:10.2f}, MAE = {mae:8.2f}")With outliers, Huber loss typically achieves the best test MAE—better than squared loss (pulled by outliers) and often competitive with or better than absolute loss (Huber's efficiency helps on clean points). Huber is often the best default choice when you're unsure about data quality.
Different libraries implement Huber loss with varying parameterizations. Understanding these differences is crucial for getting consistent results.
Scikit-learn:
from sklearn.ensemble import GradientBoostingRegressor
model = GradientBoostingRegressor(
loss='huber',
alpha=0.9, # Quantile for robust estimation of δ
n_estimators=100
)
Scikit-learn uses alpha to compute δ as a quantile of residuals. Higher alpha = larger δ = more like squared loss.
LightGBM:
import lightgbm as lgb
model = lgb.LGBMRegressor(
objective='huber',
huber_delta=1.0, # Explicit δ parameter
n_estimators=100
)
LightGBM uses a fixed huber_delta parameter.
XGBoost:
XGBoost doesn't have built-in Huber loss, but you can define it as a custom objective:
def huber_obj(preds, dtrain, delta=1.0):
labels = dtrain.get_label()
residual = preds - labels
grad = np.clip(residual, -delta, delta)
hess = (np.abs(residual) <= delta).astype(float)
return grad, hess
| Library | Parameter Name | Default Value | Notes |
|---|---|---|---|
| Scikit-learn | alpha | 0.9 | Quantile for δ estimation |
| LightGBM | huber_delta | 1.0 | Explicit δ value |
| XGBoost | (custom) | Define via custom objective | |
| CatBoost | Huber:delta | 1.0 | Explicit δ value |
Sklearn's 'alpha' is NOT the same as LightGBM's 'delta'. In sklearn, alpha=0.9 means δ is the 90th percentile of residuals. In LightGBM, delta=1.0 is the actual threshold value. Don't confuse them when porting code between libraries.
Huber loss occupies the sweet spot between squared and absolute loss. Here's guidance on when to choose it.
Use Huber Loss When:
Suspected outliers but uncertain: You think there might be outliers but aren't sure. Huber is a safe default.
Mixed error distribution: Some errors are normal (small), some are exceptional (large). Huber handles both appropriately.
Moderate contamination (5-20%): This is Huber's sweet spot. Too little contamination → squared loss is fine. Too much → consider absolute loss.
Need smooth optimization: Huber's smoothness makes optimization more stable than absolute loss.
Statistical efficiency matters: When every bit of accuracy counts on clean points, Huber's 95% efficiency beats absolute loss's ~64% efficiency.
Consider Alternatives When:
Clean data, Gaussian errors: Use squared loss for maximum efficiency.
Heavy contamination (>25%): Use absolute loss or more robust methods (trimmed, Tukey bisquare).
Confidence intervals needed: Huber doesn't have clean distributional properties like quantile regression.
Computational simplicity: Squared loss is simpler to implement and debug.
| Scenario | Recommended Loss | Reason |
|---|---|---|
| Clean data, Gaussian errors | Squared | Maximum efficiency |
| Light contamination (< 10%) | Huber | Good efficiency + robustness |
| Moderate contamination (10-25%) | Huber | Balanced approach |
| Heavy contamination (> 25%) | Absolute | Need maximum robustness |
| Unknown data quality | Huber | Safe default |
| Large errors are truly costly | Squared | Penalizes large errors strongly |
| Want median prediction | Absolute | Targets conditional median |
When in doubt, try all three—squared, Huber, and absolute—and compare on validation data. Often the difference is small, but occasionally the right choice makes a big difference. The computational cost of comparing is usually worth the potential gain.
We've thoroughly explored Huber loss as the optimal compromise between efficiency and robustness. Let's consolidate the key insights:
What's Next:
We've covered regression losses—squared, absolute, and Huber. The next page shifts to classification losses, starting with the logistic loss. Classification presents different challenges: outputs are probabilities, labels are discrete, and the loss function must handle the log-odds scale. Understanding logistic loss is essential for gradient boosting classifiers like XGBoost for classification tasks.
You now understand Huber loss as the principled, theoretically optimal compromise between squared and absolute loss. This knowledge equips you to make informed choices about loss functions in gradient boosting, selecting the right tool for your data characteristics.