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High-dimensional statistics

High-dimensional statistics is a subfield of statistics focused on the analysis of datasets where the number of variables or features (p) is large relative to the number of observations (n), often with p exceeding or comparable to n, which invalidates many classical statistical assumptions and methods designed for low-dimensional settings where np. This area addresses the inherent complexities of such , including sparsity, accumulation, and computational demands, by developing non-asymptotic theories and procedures that provide reliable even in finite samples. The roots of high-dimensional statistics trace back to early 20th-century foundational work in classical statistics, such as Fisher's methods for multivariate analysis, but gained prominence in the late 20th and early 21st centuries due to explosive growth in data from fields like and , where p can reach millions. Influential developments include random matrix theory from the 1960s and 1970s, pioneered by researchers like Vladimir Marčenko and Leonid Pastur, which provided asymptotic tools for understanding the spectral properties of high-dimensional covariance matrices. Modern frameworks, such as those emphasizing sparsity and regularization, were advanced through seminal texts like Bühlmann and van de Geer's comprehensive treatment of methods and theory for high-dimensional data. Key challenges in high-dimensional statistics include the curse of dimensionality, where the volume of the feature space grows exponentially with p, leading to sparse data coverage and inflated variance in estimators; , as traditional models like fail when p > n; and irreproducibility in applications like biomarker discovery, with studies showing up to 75% non-replication rates due to unadjusted multiple testing. These issues are compounded by the need for robust variable selection amid irrelevant noise variables and the computational infeasibility of exhaustive searches in high dimensions. Prominent methods in high-dimensional statistics revolve around regularization techniques to enforce sparsity, such as (least absolute shrinkage and selection operator) for simultaneous estimation and variable selection in linear models, and for stabilizing covariance estimates. Other approaches include adapted for high dimensions, random matrix theory-based denoising of covariance matrices, and non-asymptotic that bound errors without relying on large-sample asymptotics. These techniques often assume that only a small subset of variables (s ≪ p) are truly relevant, enabling consistent recovery through penalized likelihood frameworks. High-dimensional statistics finds critical applications in for analysis and cancer prognosis, for amid numerous assets, and in communications to handle multi-antenna systems. In , it underpins scalable algorithms for , while in , it aids in decoding high-resolution brain imaging data. Ongoing research emphasizes integrating these methods with and robustness to further advance interdisciplinary data-driven discoveries.

Definition and Motivation

Core Definition

High-dimensional statistics is the study of in settings where the dimension p (number of variables or parameters) is comparable to or larger than the sample size n, such as p \geq n or p \gg n. In this regime, classical statistical methods, which rely on assumptions like fixed p and n \to \infty, break down because the number of unknowns overwhelms the available data, leading to issues like and lack of . Central to this field is the development of non-asymptotic theory, which provides finite-sample guarantees without requiring n to grow indefinitely while keeping p fixed. Instead, analyses often consider Kolmogorov-type asymptotics, where both n and p tend to such that the p/n \to \gamma for some \gamma \in (0, \infty). This setup captures the essential challenges of high dimensions, including the curse of dimensionality, where the volume of the parameter space explodes exponentially with p. To enable reliable , high-dimensional statistics relies on structural assumptions that impose low-dimensionality on the high-dimensional objects. Key concepts include , where the true has only a small number of nonzero entries; low- structures, which assume matrices like operators have limited effective ; and regularization techniques that penalize to achieve . For instance, the general modeling framework is Y = f(X; [\theta](/page/Theta)) + \varepsilon, where [\theta](/page/Theta) \in \mathbb{R}^p is the of , \varepsilon is , and requires assumptions like \|[\theta](/page/Theta)\|_0 \leq s with level s \ll p to counteract the dimensionality.

Fundamental Challenges

One of the primary challenges in high-dimensional statistics arises from the curse of dimensionality, where the volume of the parameter space grows exponentially with the number of dimensions p, resulting in sparse data coverage relative to the space's size. This sparsity leads to instability in estimators, as the effective sample size per dimension diminishes rapidly, making it difficult to reliably estimate underlying structures or patterns without assumptions like sparsity. For instance, in nonparametric estimation, the optimal slows dramatically as p increases, exacerbating the need for or regularization techniques to mitigate this effect. Classical statistical procedures also break down in high dimensions, particularly when the dimension p is comparable to or exceeds the sample size n. The sample \hat{\Sigma}, a of multivariate , becomes inconsistent as p/n \to \alpha \in (0,1), failing to converge to the true population covariance \Sigma even as n \to \infty. This inconsistency is characterized by the Marchenko-Pastur law, which describes the asymptotic eigenvalue distribution of \hat{\Sigma} under the assumption of independent and identically distributed entries with zero and unit variance. The density function is given by f(\lambda) = \frac{1}{2\pi \alpha \lambda} \sqrt{(\lambda - a)(b - \lambda)}, where a = (1 - \sqrt{\alpha})^2 and b = (1 + \sqrt{\alpha})^2, with support [a, b] for \alpha \leq 1, illustrating how the bulk of eigenvalues concentrate in a non-degenerate interval rather than collapsing to the true eigenvalues of \Sigma. This phenomenon implies that traditional methods like or Hotelling's T^2 test lose their validity, as the largest eigenvalues of \hat{\Sigma} are inflated by noise rather than signal. In high-dimensional settings, multiple hypothesis testing poses another significant obstacle, as testing p hypotheses with only n samples increases the risk of false discoveries exponentially. Traditional control of the (FWER), which bounds the probability of any false positive, becomes overly conservative, drastically reducing power when p \gg n. To address this, the (FDR), defined as the expected proportion of false positives among rejected hypotheses, offers a more balanced approach suitable for large-scale testing. The seminal Benjamini-Hochberg procedure controls the FDR at a specified level q by sorting the p-values in ascending order and rejecting the first k hypotheses, where k is the largest index such that p_{(k)} \leq (k/p) q, with p the number of tests, enabling discovery of true signals while managing error inflation in high dimensions. Finally, hinders exact solutions in high-dimensional problems, particularly for sparsity recovery in regression models. The problem of exact subset selection—identifying the true of a sparse parameter \beta with s \ll p nonzeros—is NP-hard, as it requires solving a over \binom{p}{s} possible subsets, which grows factorially with p. This intractability necessitates heuristic or approximate algorithms, as exhaustive search becomes infeasible even for moderate p.

Historical Development

Early Foundations

The foundations of high-dimensional statistics emerged in the mid-20th century, driven by challenges in estimating parameters when the number of dimensions p exceeds or approaches the sample size n, even if p remained relatively small compared to modern scales. A pivotal insight came from Charles Stein's demonstration that the maximum likelihood estimator (MLE), specifically the sample mean \bar{y}, for the mean \mu of a p-variate N_p(\mu, I_p) is inadmissible under integrated squared error loss when p \geq 3. This result revealed that no estimator can be best for all \mu, as there exist alternatives with uniformly lower or equal risk, and strictly lower for some \mu, challenging the optimality of classical estimators in higher dimensions and motivating shrinkage techniques to reduce variance at the cost of slight bias. Building on Stein's paradox, Willard James and Charles Stein introduced in 1961 the James-Stein estimator, an empirical Bayes shrinkage method that dominates the MLE in total squared error . For estimating \mu based on observations y \sim N_p(\mu, I_p), the estimator is given by \hat{\theta}_{JS} = \left(1 - \frac{p-2}{\|\bar{y}\|^2}\right) \bar{y}, which shrinks the MLE \bar{y} toward the origin by a factor depending on p and the data's norm. This estimator achieves a risk reduction of approximately $2/p relative to the MLE when \mu = 0, and its positive-part variant further improves performance near the boundary, establishing shrinkage as a core principle for high-dimensional estimation and influencing subsequent bias-variance trade-offs. A key early advancement in understanding high-dimensional covariance structures was the Marchenko–Pastur law, developed by Vladimir Marchenko and Leonid Pastur in 1967. This result describes the of eigenvalues of the sample when both p and n grow such that p/n \to \gamma \in (0, \infty), revealing a bulk spectrum that deviates from the classical fixed-p case and highlighting phenomena like the largest eigenvalue's , which informs denoising and inference in high dimensions. In the context of linear regression, Arthur Hoerl and Robert Kennard proposed in 1970 to address instability due to , a common issue when p nears n. The ridge estimator solves the penalized problem \hat{\beta}_{\text{ridge}} = \arg\min_{\beta} \|Y - X\beta\|^2_2 + \lambda \|\beta\|^2_2, where \lambda > 0 is a tuning parameter controlling the penalty. By adding a ridge to the X^T X, it stabilizes coefficient estimates and reduces in scenarios with near-singular design matrices, laying groundwork for regularized methods in near-high-dimensional settings without assuming sparsity. Early theoretical support for handling covariance structures in higher dimensions drew from random matrix theory, particularly the introduced by John Wishart in , which describes the distribution of the sample S = \sum_{i=1}^n (x_i - \bar{x})(x_i - \bar{x})^T for n i.i.d. observations x_i \sim N_p([\mu, \Sigma](/page/Mu_Sigma)). In the classical regime where p is fixed and n \to \infty (so p/n \to 0), asymptotic results show that n S converges in distribution to a W_p(n, \Sigma), with the eigenvalues of S concentrating around those of \Sigma, enabling consistent inference on population covariances and providing limits that informed later high-dimensional extensions.

Key Milestones in Modern Era

The introduction of the by in 1996 marked a pivotal shift toward sparsity-inducing methods in high-dimensional . The estimator is defined as \hat{\beta}_{\text{lasso}} = \arg\min_{\beta} \|Y - X\beta\|^2 + \lambda \|\beta\|_1, where \lambda > 0 is a tuning parameter that balances fit and sparsity. This \ell_1-penalized approach promotes variable selection by shrinking some coefficients to exactly zero through soft-thresholding, addressing the limitations of earlier shrinkage methods like that only shrink but do not select variables. The method's ability to perform simultaneous estimation and selection in settings where the number of predictors exceeds the sample size has made it foundational for modern high-dimensional statistics. In the 2000s, developments in by David Donoho, Emmanuel Candès, and provided theoretical foundations that paralleled and reinforced sparsity-based recovery in statistics. These works established conditions under which s-sparse signals can be exactly recovered from underdetermined linear measurements using \ell_1 minimization, akin to . A key innovation was the (RIP), which ensures that the sensing matrix preserves the geometry of sparse vectors, allowing stable recovery with high probability when the number of measurements is on the order of s \log(p/s), where p is the ambient . This framework not only bridged and statistics but also inspired rigorous guarantees for sparse in high dimensions, emphasizing the role of incoherence and compatibility conditions. Advances in theory during the , particularly by Afonso Bandeira and Ramon van Handel, sharpened non-asymptotic bounds essential for high-dimensional estimation. Their work derived optimal rates for the spectral norm of random matrices with independent entries, providing tools to control operator norms in sparse settings without relying on asymptotic assumptions. These bounds imply improved error rates for estimation under sparsity, such as achieving rates of order \sqrt{ \frac{s \log p}{n} } for s-sparse matrices. Such results have been instrumental in scaling statistical procedures to massive datasets while maintaining theoretical . Post-2020 trends have increasingly integrated high-dimensional statistics with , exemplified by the double/debiased (DML) framework developed by Victor Chernozhukov and collaborators starting in 2018, with ongoing refinements through 2023. DML enables robust in high dimensions by combining flexible for nuisance parameters with debiased corrections to achieve \sqrt{n}- for low-dimensional targets, even when the dimension grows with n. Updates in recent years have extended DML to handle heterogeneous treatment effects and integrated it with advanced learners like random forests, facilitating applications in and beyond. This synthesis underscores the field's evolution toward scalable, inference-valid methods in the era.

Core Methodological Topics

Sparse Regression and Variable Selection

Sparse regression methods address the challenge of estimating regression coefficients in high-dimensional linear models Y = X\beta + \epsilon, where the number of features p greatly exceeds the sample size n, by imposing sparsity assumptions that only s \ll p coefficients in \beta are non-zero. The (Least Absolute Shrinkage and Selection Operator) is a foundational approach, formulated as the \hat{\beta} = \arg\min_{\beta} \frac{1}{2n} \|Y - X\beta\|_2^2 + \lambda \|\beta\|_1, which simultaneously performs estimation and variable selection by shrinking irrelevant coefficients to zero through the \ell_1 penalty. Key theoretical properties of the Lasso include oracle inequalities bounding the prediction error. Specifically, under the restricted eigenvalue condition on the X, the Lasso estimator satisfies \frac{\|X(\hat{\beta} - \beta^*)\|_2^2}{n} \leq C \frac{s \log p}{n} \sigma^2 with high probability, where \beta^* is the true sparse parameter, s is its sparsity level, \sigma^2 is the noise variance, and C > 0 is a constant. For variable selection consistency, the irrepresentable condition must hold, which requires that the columns of X corresponding to inactive predictors (zero coefficients in \beta^*) are not strongly correlated with those of active predictors, ensuring exact of the support of \beta^*. Achieving these consistency guarantees typically involves tuning the regularization parameter \lambda on the order of \sigma \sqrt{\log p / n}, balancing and variance in the high-dimensional regime. Despite its strengths, the Lasso can introduce bias toward zero for large coefficients due to the convex \ell_1 penalty. To address this, the adaptive Lasso refines the penalty by incorporating data-dependent weights, solving \hat{\beta} = \arg\min_{\beta} \frac{1}{2n} \|Y - X\beta\|_2^2 + \lambda \sum_{j=1}^p w_j |\beta_j|, where w_j = 1 / |\hat{\beta}_j^{\text{init}}|^\gamma for some initial \hat{\beta}^{\text{init}} (often ) and \gamma > 0. This weighting promotes stronger shrinkage for small coefficients while preserving large ones, yielding oracle properties: consistent and asymptotic normality as if the true were known. Non-convex penalties offer further improvements in unbiasedness for significant effects. The smoothly clipped deviation (SCAD) penalty, defined as p(\theta) = \lambda |\theta| for |\theta| \leq \lambda, p(\theta) = a\lambda |\theta| - (\theta - \lambda)^2 / (2(a-1)) for \lambda < |\theta| \leq a\lambda, and constant thereafter, reduces bias for large |\theta| while enforcing sparsity, and is optimized via local quadratic approximation. Similarly, the minimax concave penalty (MCP), given by p(\theta) = \lambda |\theta| - \theta^2 / (2b) for |\theta| \leq b\lambda and \lambda^2 b / 2 otherwise, achieves nearly unbiased estimation in sparse regions by maximizing concavity under constraints for selection and unbiasedness thresholds. For scenarios with structured sparsity, where non-zero coefficients cluster in predefined groups (e.g., genes in pathways), the group Lasso extends the framework to \hat{\beta} = \arg\min_{\beta} \frac{1}{2n} \|Y - X\beta\|_2^2 + \lambda \sum_{g=1}^G \|\beta_g\|_2, penalizing the \ell_2 norm of each group \beta_g to select or shrink entire groups to zero. This is particularly effective for overlapping groups in , such as shared genetic variants across traits, enabling joint modeling while respecting biological structure. Theoretical guarantees for these methods include model selection consistency, where the estimator \hat{\beta} recovers the true support with probability approaching one. For the Lasso, this holds under conditions like the irrepresentable or restricted eigenvalue assumptions, with the \ell_1-error bounded as \|\hat{\beta} - \beta^*\|_1 \leq C s \lambda for some constant C > 0, ensuring tight recovery in the high-dimensional limit.

and Precision Matrix Estimation

In high-dimensional settings where the number of variables p exceeds the sample size n, the sample \hat{\Sigma} = \frac{1}{n} X^T X (with X centered) becomes singular and inconsistent as an estimator of the true \Sigma, leading to poor performance in downstream tasks like or . Specifically, under mild conditions on the entries of \Sigma, the expected loss \mathbb{E} \|\hat{\Sigma} - \Sigma\|_F^2 grows with p, diverging as p/n \to c > 0. Moreover, the extreme eigenvalues of \hat{\Sigma} exhibit non-degenerate limiting behavior governed by random matrix theory: the largest eigenvalue, properly scaled, converges in distribution to the Tracy-Widom law when p/n \to \gamma \in (0,1), highlighting systematic away from the population eigenvalues. To address these issues, shrinkage estimators combine the sample covariance with a structured target matrix, improving conditioning and reducing variance. A seminal approach is the Ledoit-Wolf estimator, which shrinks towards a scaled identity matrix: \hat{\Sigma}_{\text{shrink}} = (1 - \phi) \hat{\Sigma} + \phi \mu I, where \mu is the average variance and \phi is the shrinkage intensity. The optimal \phi minimizes the expected quadratic loss and is asymptotically given by \phi = \frac{\operatorname{tr}(\Sigma - \hat{\Sigma})^2}{\|\Sigma - \hat{\Sigma}\|_F^2}, achieving consistency in the Frobenius norm as long as p/n \to 0 or under bounded effective dimension. This method outperforms the sample covariance in high dimensions by balancing bias and variance, with empirical advantages in applications requiring well-conditioned matrices. Precision matrix estimation, where \Omega = \Sigma^{-1} encodes conditional independencies in Gaussian graphical models, exploits sparsity to handle high dimensionality. In these models, zero entries in \Omega correspond to absent edges in the , allowing row-wise techniques to recover structure. The neighborhood selection method treats each row of \Omega as a sparse problem, applying the penalty: for variable j, regress X_j on the other variables and select non-zero coefficients as neighbors. Under the neighborhood stability condition (ensuring sparse partial correlations), this approach consistently estimates the with high probability when the maximum degree d satisfies d \log p / n \to 0. This ties briefly to sparse techniques by leveraging \ell_1 penalties per row, but focuses on undirected recovery rather than vector selection. For covariances exhibiting low-rank structure, nuclear norm minimization provides a convex relaxation to enforce rank constraints while estimating \Sigma. The estimator solves \min_{\Theta \succeq 0} \|\Theta\|_* + \lambda \|\Theta - \hat{\Sigma}\|_F^2, or more generally, \min \|\Theta\|_* subject to observation constraints, where \|\cdot\|_* is the sum of singular values. For a rank-r \Sigma observed through n samples, this achieves a convergence rate of O(\sqrt{r p / n}) in the Frobenius norm under incoherence conditions, outperforming unstructured estimators by exploiting the effective dimension r p. Such methods are particularly effective when the signal concentrates in few principal components, as in factor models.

High-Dimensional Inference and Testing

In high-dimensional statistics, inference and testing procedures must account for the challenges posed by the dimensionality exceeding the sample size, such as inflated type I errors and invalid confidence intervals due to model selection or multiple comparisons. Traditional methods assuming low dimensionality often fail, necessitating specialized techniques that control error rates while maintaining power. Key approaches include multiple testing corrections, post-selection inference frameworks, high-dimensional central limit theorems for approximation guarantees, and debiasing methods for estimators like the Lasso. These tools enable valid hypothesis testing and uncertainty quantification in sparse, high-dimensional settings. Multiple testing control is essential in high dimensions, where thousands of hypotheses may be tested simultaneously, leading to a high of false positives. The Benjamini-Hochberg procedure addresses this by controlling the (FDR), defined as the expected proportion of false rejections among all rejections, at a level q. The method involves sorting the m p-values in ascending order as p_{(1)} \leq p_{(2)} \leq \cdots \leq p_{(m)}, then finding the largest k such that p_{(k)} \leq (k/m) q, and rejecting all hypotheses with p-values up to p_{(k)}. Under or positive dependence of test statistics, this procedure ensures FDR \leq q. Post-selection provides a framework for valid p-values and confidence intervals after variable selection, avoiding the pitfalls of naive application of standard tests on selected models. The selective approach, applied to methods like the for sparse , conditions on the selection event to construct truncated likelihoods. Specifically, for the , the post-selection distribution of a selected follows a truncated Gaussian, enabling exact by solving a polyhedral optimization to determine the truncation region. This yields pivotal quantities for testing and intervals that account for , maintaining type I error control conditional on selection. High-dimensional central limit theorems (CLTs) underpin many inference procedures by justifying Gaussian approximations for statistics like maxima over coordinates, despite p \gg n. Berry-Esseen-type bounds quantify the approximation error for the distribution of \max_j Z_{n,j}, where Z_{n,j} = \sqrt{n} (\bar{Y}_j - \mu_j)/\sigma_j are normalized sample means. Under sub-Gaussian tails and sparsity, the supremum over t of the difference between the CDF of \max_j Z_{n,j} and that of a Gaussian maximum satisfies \sup_t |P(\max_j Z_{n,j} \leq t) - \Lambda_p(t)| \leq C (\log p)^{7/6} / n^{1/6}, where \Lambda_p is the CDF of the maximum of p standard normals and C is a constant. This bound enables uniform inference over coordinates, such as simultaneous confidence bands. The desparsified extends inference to individual coefficients in high-dimensional linear models by debiasing the standard estimator, which is selection-consistent but asymptotically biased under sparsity. The debiased estimator is given by \hat{\beta}^{\text{deb}}_{j} = \hat{\beta}^{\text{lasso}}_j + \frac{1}{n} \frac{X_j^T (Y - X \hat{\beta}^{\text{lasso}})}{\hat{\Gamma}_{jj}}, where \hat{\Gamma} estimates the inverse of the features, often via nodewise regressions. Under irrepresentable conditions and s \log p / n \to 0 (with s the sparsity level), \sqrt{n} (\hat{\beta}^{\text{deb}}_j - \beta_j) converges to a with mean zero and variance \sigma^2 / \hat{\Gamma}_{jj}, allowing construction of asymptotically valid confidence intervals and t-tests for \beta_j. This approach builds on the as a selection tool while correcting for its shrinkage.

Applications and Examples

Linear Models and Parameter Estimation

In high-dimensional linear regression, the model is typically formulated as Y_i = x_i^T \beta + \varepsilon_i for i=1,\dots,n, where Y_i is the response, x_i \in \mathbb{R}^p is a of predictors, \beta \in \mathbb{R}^p is the sparse with at most s nonzero entries (s \ll p), and \varepsilon_i are errors with zero and constant variance. When p \gg n, ordinary least squares (OLS) estimation \hat{\beta}_{\text{OLS}} = (X^T X)^{-1} X^T Y becomes unstable or undefined, as the X \in \mathbb{R}^{n \times p} leads to a singular or ill-conditioned X^T X, resulting in high variance and . To address this, the Lasso estimator applies \ell_1 regularization: \hat{\beta}_{\text{lasso}} = \arg\min_{\beta} \frac{1}{2n} \|Y - X\beta\|_2^2 + \lambda \|\beta\|_1, where \lambda > 0 controls sparsity. The tuning parameter \lambda is commonly selected via cross-validation to minimize prediction error on held-out data. Under the irrepresentable condition on the design matrix—requiring that the columns corresponding to zero coefficients in \beta cannot be well-approximated by those of the active set—Lasso achieves sign consistency, meaning P(\text{sign}(\hat{\beta}_{\text{lasso}}) = \text{sign}(\beta)) \to 1 as n \to \infty when s = o(\sqrt{n}) and \lambda is chosen appropriately. (For broader Lasso theory, see the section on Sparse Regression and Variable Selection.) Simulation studies illustrate 's performance relative to in recovering sparse signals amid correlated predictors. tends to achieve higher true positive rates and lower false positives compared to , which retains all variables and can suffer from diffusion in such settings. also often yields lower on test sets when the true \beta is sparse, as 's \ell_2 penalty shrinks coefficients uniformly without selection, leading to higher in correlated settings. An empirical illustration arises in analysis, where selects top biomarkers from datasets with p \approx 20,000 genes and n \approx 100 samples, such as those from experiments classifying cancer subtypes. In such cases, identifies a small set of influential genes (e.g., 20-50 nonzero coefficients) that predict outcomes like survival, outperforming unregularized methods by reducing noise from irrelevant features and improving model interpretability.

Real-World Domains

High-dimensional statistics has found extensive applications in genomics, where datasets often feature millions of single nucleotide polymorphisms (SNPs) as predictors (p in the millions) and thousands of samples (n in the thousands), necessitating sparse methods to identify meaningful patterns amid noise. In gene clustering tasks, sparse principal component analysis (sparse PCA) enables the extraction of interpretable principal components by enforcing sparsity on loadings, thus selecting a subset of genes that capture variance while facilitating biological insights. For instance, sparse PCA applied to colon cancer microarray data (p=2,000 genes, n=62 samples) reduced the feature set to 13 genes while achieving a clustering Rand index of 0.669, comparable to standard PCA's 0.654, and overlapping with seven key genes identified by recursive feature elimination-support vector machines. Similarly, in lymphoma datasets, it selected 108 genes for robust clustering. For expression quantitative trait loci (eQTL) mapping, which links SNPs to gene expression levels, the Lasso and its extensions address the high-dimensional challenge by imposing sparsity to detect regulatory variants. The tree-guided group Lasso, for example, incorporates hierarchical SNP structures to estimate multi-response regressions, demonstrating superior performance in simulated eQTL data with around 200 covariates and 150 samples, recovering true associations with higher precision than independent Lasso. In , high-dimensional methods are crucial for managing portfolios with hundreds of assets (p >> n trading days), particularly in where data volumes explode. estimation under such regimes leverages thresholding and factor models to handle noise and heteroscedasticity in intraday returns, enabling minimum variance . A key approach, the principal orthogonal complement thresholding () method, estimates large from factor models, applied to equity portfolios and yielding improved out-of-sample performance over sample covariance benchmarks by reducing error. For risk factor models, precision matrix via graphical models uncovers conditional independencies among assets, informing sparse risk assessments. The factor graphical decomposes the precision matrix into a low-rank factor component and a sparse idiosyncratic part, proven consistent under spectral norms for heavy-tailed returns; in applications (p=500 assets), it improved global minimum variance portfolio returns by 10-15% out-of-sample compared to estimators. Integration with highlights high-dimensional statistics in for tasks like image , where pixel features (p=784 for MNIST digits) scale to millions in larger datasets, requiring sparsity to combat of dimensionality. Lasso-based methods select relevant features by penalizing irrelevant coefficients, enhancing classifier accuracy; for instance, sure independence screening followed by on high-dimensional image data reduces features from thousands to dozens, achieving errors below 5% on benchmark datasets by prioritizing discriminative pixels. In recommender systems, addresses incomplete user-item matrices (p and n in millions, with 99% missing entries), approximating low-rank structures to predict preferences. During the , matrix factorization techniques completed rating matrices for 480,000 users and 17,000 movies, improving error by 9.5% over baselines through latent factor estimation, with regularized models handling high-dimensional sparsity effectively. Post-2020 advancements include in using double machine learning (double ML) to estimate treatment effects amid high-dimensional confounders (p >> n), such as in policy evaluations with numerous covariates. Double ML debiases nuisance parameters via cross-fitting machine learning estimators (e.g., random forests), enabling root-n consistent inference; an extension for continuous treatments demonstrated improved estimation in simulations. This approach has been adapted for panels with fixed effects in subsequent work, providing robust inference in high-dimensional settings like analyses with thousands of macro variables.

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    Recommender systems rely on different types of input data, which are often placed in a matrix with one dimension representing users and the other dimension.Missing: completion | Show results with:completion
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    This paper proposes a nonparametric method using double debiased machine learning (DML) to estimate causal effects of continuous treatments, using a doubly ...