近似贝叶斯深度学习方法对于解决在智能系统中部署深度学习组件时，包括在智能系统中部署深度学习组件的几个问题，包括减轻过度自信的错误并提供增强的鲁棒性，从而超出分发示例。但是，现有近似贝叶斯推理方法的计算要求可以使它们不适合部署包括低功耗边缘设备的智能IOT系统。在本文中，我们为监督深度学习提供了一系列近似贝叶斯推理方法，并在应用这些方法对当前边缘硬件上的挑战和机遇。我们突出了几种潜在的解决方案来降低模型存储要求，提高计算可扩展性，包括模型修剪和蒸馏方法。

While machine learning is traditionally a resource intensive task, embedded systems, autonomous navigation, and the vision of the Internet of Things fuel the interest in resource-efficient approaches. These approaches aim for a carefully chosen trade-off between performance and resource consumption in terms of computation and energy. The development of such approaches is among the major challenges in current machine learning research and key to ensure a smooth transition of machine learning technology from a scientific environment with virtually unlimited computing resources into everyday's applications. In this article, we provide an overview of the current state of the art of machine learning techniques facilitating these real-world requirements. In particular, we focus on deep neural networks (DNNs), the predominant machine learning models of the past decade. We give a comprehensive overview of the vast literature that can be mainly split into three non-mutually exclusive categories: (i) quantized neural networks, (ii) network pruning, and (iii) structural efficiency. These techniques can be applied during training or as post-processing, and they are widely used to reduce the computational demands in terms of memory footprint, inference speed, and energy efficiency. We also briefly discuss different concepts of embedded hardware for DNNs and their compatibility with machine learning techniques as well as potential for energy and latency reduction. We substantiate our discussion with experiments on well-known benchmark datasets using compression techniques (quantization, pruning) for a set of resource-constrained embedded systems, such as CPUs, GPUs and FPGAs. The obtained results highlight the difficulty of finding good trade-offs between resource efficiency and predictive performance.

现代深度学习方法构成了令人难以置信的强大工具，以解决无数的挑战问题。然而，由于深度学习方法作为黑匣子运作，因此与其预测相关的不确定性往往是挑战量化。贝叶斯统计数据提供了一种形式主义来理解和量化与深度神经网络预测相关的不确定性。本教程概述了相关文献和完整的工具集，用于设计，实施，列车，使用和评估贝叶斯神经网络，即使用贝叶斯方法培训的随机人工神经网络。

量化监督学习模型的不确定性在制定更可靠的预测方面发挥着重要作用。认知不确定性，通常是由于对模型的知识不足，可以通过收集更多数据或精炼学习模型来减少。在过去的几年里，学者提出了许多认识的不确定性处理技术，这些技术可以大致分为两类，即贝叶斯和集合。本文对过去五年来提供了对监督学习的认识性不确定性学习技术的全面综述。因此，我们首先，将认知不确定性分解为偏见和方差术语。然后，介绍了认知不确定性学习技术以及其代表模型的分层分类。此外，提出了几种应用，例如计算机视觉（CV）和自然语言处理（NLP），然后讨论研究差距和可能的未来研究方向。

We propose SWA-Gaussian (SWAG), a simple, scalable, and general purpose approach for uncertainty representation and calibration in deep learning. Stochastic Weight Averaging (SWA), which computes the first moment of stochastic gradient descent (SGD) iterates with a modified learning rate schedule, has recently been shown to improve generalization in deep learning. With SWAG, we fit a Gaussian using the SWA solution as the first moment and a low rank plus diagonal covariance also derived from the SGD iterates, forming an approximate posterior distribution over neural network weights; we then sample from this Gaussian distribution to perform Bayesian model averaging. We empirically find that SWAG approximates the shape of the true posterior, in accordance with results describing the stationary distribution of SGD iterates. Moreover, we demonstrate that SWAG performs well on a wide variety of tasks, including out of sample detection, calibration, and transfer learning, in comparison to many popular alternatives including MC dropout, KFAC Laplace, SGLD, and temperature scaling.

The success of machine learning algorithms generally depends on data representation, and we hypothesize that this is because different representations can entangle and hide more or less the different explanatory factors of variation behind the data. Although specific domain knowledge can be used to help design representations, learning with generic priors can also be used, and the quest for AI is motivating the design of more powerful representation-learning algorithms implementing such priors. This paper reviews recent work in the area of unsupervised feature learning and deep learning, covering advances in probabilistic models, auto-encoders, manifold learning, and deep networks. This motivates longer-term unanswered questions about the appropriate objectives for learning good representations, for computing representations (i.e., inference), and the geometrical connections between representation learning, density estimation and manifold learning.

We propose a simultaneous learning and pruning algorithm capable of identifying and eliminating irrelevant structures in a neural network during the early stages of training. Thus, the computational cost of subsequent training iterations, besides that of inference, is considerably reduced. Our method, based on variational inference principles using Gaussian scale mixture priors on neural network weights, learns the variational posterior distribution of Bernoulli random variables multiplying the units/filters similarly to adaptive dropout. Our algorithm, ensures that the Bernoulli parameters practically converge to either 0 or 1, establishing a deterministic final network. We analytically derive a novel hyper-prior distribution over the prior parameters that is crucial for their optimal selection and leads to consistent pruning levels and prediction accuracy regardless of weight initialization or the size of the starting network. We prove the convergence properties of our algorithm establishing theoretical and practical pruning conditions. We evaluate the proposed algorithm on the MNIST and CIFAR-10 data sets and the commonly used fully connected and convolutional LeNet and VGG16 architectures. The simulations show that our method achieves pruning levels on par with state-of the-art methods for structured pruning, while maintaining better test-accuracy and more importantly in a manner robust with respect to network initialization and initial size.

变异推理（VI）的核心原理是将计算复杂后概率密度计算的统计推断问题转换为可拖动的优化问题。该属性使VI比几种基于采样的技术更快。但是，传统的VI算法无法扩展到大型数据集，并且无法轻易推断出越野数据点，而无需重新运行优化过程。该领域的最新发展，例如随机，黑框和摊销VI，已帮助解决了这些问题。如今，生成的建模任务广泛利用摊销VI来实现其效率和可扩展性，因为它利用参数化函数来学习近似的后验密度参数。在本文中，我们回顾了各种VI技术的数学基础，以构成理解摊销VI的基础。此外，我们还概述了最近解决摊销VI问题的趋势，例如摊销差距，泛化问题，不一致的表示学习和后验崩溃。最后，我们分析了改善VI优化的替代差异度量。

Normalizing flows provide a general mechanism for defining expressive probability distributions, only requiring the specification of a (usually simple) base distribution and a series of bijective transformations. There has been much recent work on normalizing flows, ranging from improving their expressive power to expanding their application. We believe the field has now matured and is in need of a unified perspective. In this review, we attempt to provide such a perspective by describing flows through the lens of probabilistic modeling and inference. We place special emphasis on the fundamental principles of flow design, and discuss foundational topics such as expressive power and computational trade-offs. We also broaden the conceptual framing of flows by relating them to more general probability transformations. Lastly, we summarize the use of flows for tasks such as generative modeling, approximate inference, and supervised learning.

Recent advances in coreset methods have shown that a selection of representative datapoints can replace massive volumes of data for Bayesian inference, preserving the relevant statistical information and significantly accelerating subsequent downstream tasks. Existing variational coreset constructions rely on either selecting subsets of the observed datapoints, or jointly performing approximate inference and optimizing pseudodata in the observed space akin to inducing points methods in Gaussian Processes. So far, both approaches are limited by complexities in evaluating their objectives for general purpose models, and require generating samples from a typically intractable posterior over the coreset throughout inference and testing. In this work, we present a black-box variational inference framework for coresets that overcomes these constraints and enables principled application of variational coresets to intractable models, such as Bayesian neural networks. We apply our techniques to supervised learning problems, and compare them with existing approaches in the literature for data summarization and inference.

One of the core problems of modern statistics is to approximate difficult-to-compute probability densities. This problem is especially important in Bayesian statistics, which frames all inference about unknown quantities as a calculation involving the posterior density. In this paper, we review variational inference (VI), a method from machine learning that approximates probability densities through optimization. VI has been used in many applications and tends to be faster than classical methods, such as Markov chain Monte Carlo sampling. The idea behind VI is to first posit a family of densities and then to find the member of that family which is close to the target. Closeness is measured by Kullback-Leibler divergence. We review the ideas behind mean-field variational inference, discuss the special case of VI applied to exponential family models, present a full example with a Bayesian mixture of Gaussians, and derive a variant that uses stochastic optimization to scale up to massive data. We discuss modern research in VI and highlight important open problems. VI is powerful, but it is not yet well understood. Our hope in writing this paper is to catalyze statistical research on this class of algorithms.

贝叶斯神经网络和深度集合代表了深入学习中不确定性量化的两种现代范式。然而，这些方法主要因内存低效率问题而争取，因为它们需要比其确定性对应物高出几倍的参数储存。为了解决这个问题，我们使用少量诱导重量增强每层的重量矩阵，从而将不确定性定量突出到这种低尺寸空间中。我们进一步扩展了Matheron的有条件高斯采样规则，以实现快速的重量采样，这使得我们的推理方法能够与合并相比保持合理的运行时间。重要的是，我们的方法在具有完全连接的神经网络和RESNET的预测和不确定性估算任务中实现了竞争性能，同时将参数大小减少到$单辆$ \ LEQ 24.3 \％$的参数大小神经网络。

我们提出了一种新的方法，可以在复杂模型（例如贝叶斯神经网络）中执行近似贝叶斯推断。该方法比马尔可夫链蒙特卡洛更可扩展到大数据，它具有比变异推断更具表现力的模型，并且不依赖于对抗训练（或密度比估计）。我们采用了构建两个模型的最新方法：（1）一个主要模型，负责执行回归或分类； （2）一个辅助，表达的（例如隐式）模型，该模型定义了主模型参数上的近似后验分布。但是，我们根据后验预测分布的蒙特卡洛估计值通过梯度下降来优化后验模型的参数 - 这是我们唯一的近似值（除后模型除外）。只需要指定一个可能性，可以采用各种形式，例如损失功能和合成可能性，从而提供无可能的方法的形式。此外，我们制定了该方法，使后样品可以独立于或有条件地取决于主要模型的输入。后一种方法被证明能够增加主要模型的明显复杂性。我们认为这在诸如替代和基于物理的模型之类的应用中很有用。为了促进贝叶斯范式如何提供不仅仅是不确定性量化的方式，我们证明了：不确定性量化，多模式以及具有最新预测的神经网络体系结构的应用。

贝叶斯范式有可能解决深度神经网络的核心问题，如校准和数据效率低差。唉，缩放贝叶斯推理到大量的空间通常需要限制近似。在这项工作中，我们表明它足以通过模型权重的小子集进行推动，以便获得准确的预测后断。另一个权重被保存为点估计。该子网推断框架使我们能够在这些子集上使用表现力，否则难以相容的后近近似。特别是，我们将子网线性化LAPLACE作为一种简单，可扩展的贝叶斯深度学习方法：我们首先使用线性化的拉普拉斯近似来获得所有重量的地图估计，然后在子网上推断出全协方差高斯后面。我们提出了一个子网选择策略，旨在最大限度地保护模型的预测性不确定性。经验上，我们的方法对整个网络的集合和较少的表达后近似进行了比较。

We present the GPry algorithm for fast Bayesian inference of general (non-Gaussian) posteriors with a moderate number of parameters. GPry does not need any pre-training, special hardware such as GPUs, and is intended as a drop-in replacement for traditional Monte Carlo methods for Bayesian inference. Our algorithm is based on generating a Gaussian Process surrogate model of the log-posterior, aided by a Support Vector Machine classifier that excludes extreme or non-finite values. An active learning scheme allows us to reduce the number of required posterior evaluations by two orders of magnitude compared to traditional Monte Carlo inference. Our algorithm allows for parallel evaluations of the posterior at optimal locations, further reducing wall-clock times. We significantly improve performance using properties of the posterior in our active learning scheme and for the definition of the GP prior. In particular we account for the expected dynamical range of the posterior in different dimensionalities. We test our model against a number of synthetic and cosmological examples. GPry outperforms traditional Monte Carlo methods when the evaluation time of the likelihood (or the calculation of theoretical observables) is of the order of seconds; for evaluation times of over a minute it can perform inference in days that would take months using traditional methods. GPry is distributed as an open source Python package (pip install gpry) and can also be found at https://github.com/jonaselgammal/GPry.

We develop an optimization algorithm suitable for Bayesian learning in complex models. Our approach relies on natural gradient updates within a general black-box framework for efficient training with limited model-specific derivations. It applies within the class of exponential-family variational posterior distributions, for which we extensively discuss the Gaussian case for which the updates have a rather simple form. Our Quasi Black-box Variational Inference (QBVI) framework is readily applicable to a wide class of Bayesian inference problems and is of simple implementation as the updates of the variational posterior do not involve gradients with respect to the model parameters, nor the prescription of the Fisher information matrix. We develop QBVI under different hypotheses for the posterior covariance matrix, discuss details about its robust and feasible implementation, and provide a number of real-world applications to demonstrate its effectiveness.

随机梯度马尔可夫链蒙特卡洛（SGMCMC）被认为是大型模型（例如贝叶斯神经网络）中贝叶斯推断的金标准。由于从业人员在这些模型中面临速度与准确性权衡，因此变异推理（VI）通常是可取的选择。不幸的是，VI对后部的分解和功能形式做出了有力的假设。在这项工作中，我们提出了一个新的非参数变分近似，该近似没有对后验功能形式进行假设，并允许从业者指定算法应尊重或断裂的确切依赖性。该方法依赖于在修改的能量函数上运行的新的langevin型算法，其中潜在变量的一部分是在马尔可夫链的早期迭代中平均的。这样，统计依赖性可以以受控的方式破裂，从而使链条混合更快。可以以“辍学”方式进一步修改该方案，从而导致更大的可扩展性。我们在CIFAR-10，SVHN和FMNIST上测试RESNET-20的计划。在所有情况下，与SG-MCMC和VI相比，我们都会发现收敛速度和/或最终精度的提高。

利用深度神经网络在监督学习设置中产生校准预测概率的多种技术已经出现了利用在多个随机起点（深坐标）的循环训练或培训期间发现的集合不同解决方案的方法。但是，只有有限的工作已经调查了探索各种解决方案（后模式）探索本地区域的效用。在CIFAR-10数据集上使用三种众所周知的深层架构，我们评估了几种简单的方法，用于探索重量空间的局部区域，相对于BRICR得分，准确性和预期的校准误差。我们考虑贝叶斯推理技术（变分推理和汉密尔顿蒙特卡罗施加到Softmax输出层）以及利用Optima附近的随机梯度下降轨迹。在将单独模式添加到合奏中均匀提高性能时，我们表明，这里考虑的简单模式探索方法在没有模式探索的情况下对整体产生的简单模式勘探方法很少。

基于采样的推理技术是现代宇宙学数据分析的核心;然而，这些方法与维度不良，通常需要近似或顽固的可能性。在本文中，我们描述了截短的边际神经比率估计（TMNRE）（即所谓的基于模拟的推断的新方法）自然避免了这些问题，提高了$（i）$效率，$（ii）$可扩展性和$ （iii）推断后的后续后续的可信度。使用宇宙微波背景（CMB）的测量，我们表明TMNRE可以使用比传统马尔可夫链蒙特卡罗（MCMC）方法更少模拟器呼叫的数量级来实现融合的后海后。值得注意的是，所需数量的样本有效地独立于滋扰参数的数量。此外，称为\ MEMPH {本地摊销}的属性允许对基于采样的方法无法访问的严格统计一致性检查的性能。 TMNRE承诺成为宇宙学数据分析的强大工具，特别是在扩展宇宙学的背景下，其中传统的基于采样的推理方法所需的时间级数融合可以大大超过$ \ Lambda $ CDM等简单宇宙学模型的时间。为了执行这些计算，我们使用开源代码\ texttt {swyft}来使用TMNRE的实现。

在这项工作中，我们使用变分推论来量化无线电星系分类的深度学习模型预测的不确定性程度。我们表明，当标记无线电星系时，个体测试样本的模型后差水平与人类不确定性相关。我们探讨了各种不同重量前沿的模型性能和不确定性校准，并表明稀疏事先产生更良好的校准不确定性估计。使用单个重量的后部分布，我们表明我们可以通过从最低信噪比（SNR）中除去权重来修剪30％的完全连接的层权重，而无需显着损失性能。我们证明，可以使用基于Fisher信息的排名来实现更大程度的修剪，但我们注意到两种修剪方法都会影响Failaroff-Riley I型和II型无线电星系的不确定性校准。最后，我们表明，与此领域的其他工作相比，我们经历了冷的后效，因此后部必须缩小后加权以实现良好的预测性能。我们检查是否调整成本函数以适应模型拼盘可以弥补此效果，但发现它不会产生显着差异。我们还研究了原则数据增强的效果，并发现这改善了基线，而且还没有弥补观察到的效果。我们将其解释为寒冷的后效，因为我们的培训样本过于有效的策划导致可能性拼盘，并将其提高到未来无线电银行分类的潜在问题。