annotate writeup/aistats2011_cameraready.tex @ 631:510220effb14

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author Yoshua Bengio <bengioy@iro.umontreal.ca>
date Sat, 19 Mar 2011 22:44:53 -0400
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1 %\documentclass[twoside,11pt]{article} % For LaTeX2e
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2 \documentclass{article} % For LaTeX2e
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3 \usepackage[accepted]{aistats2e_2011}
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4 %\usepackage{times}
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5 \usepackage{wrapfig}
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6 \usepackage{amsthm}
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7 \usepackage{amsmath}
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8 \usepackage{bbm}
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9 \usepackage[utf8]{inputenc}
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10 \usepackage[psamsfonts]{amssymb}
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11 %\usepackage{algorithm,algorithmic} % not used after all
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12 \usepackage{graphicx,subfigure}
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13 \usepackage{natbib}
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15 \addtolength{\textwidth}{10mm}
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16 \addtolength{\evensidemargin}{-5mm}
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17 \addtolength{\oddsidemargin}{-5mm}
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18
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19 %\setlength\parindent{0mm}
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21 \begin{document}
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22
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23 \twocolumn[
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24 \aistatstitle{Deep Learners Benefit More from Out-of-Distribution Examples}
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25 \runningtitle{Deep Learners for Out-of-Distribution Examples}
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26 \runningauthor{Bengio et. al.}
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27 \aistatsauthor{
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28 Yoshua Bengio \and
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29 Frédéric Bastien \and
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30 \bf Arnaud Bergeron \and
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31 Nicolas Boulanger-Lewandowski \and \\
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32 \bf Thomas Breuel \and
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33 Youssouf Chherawala \and
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34 \bf Moustapha Cisse \and
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35 Myriam Côté \and \\
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36 \bf Dumitru Erhan \and
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37 Jeremy Eustache \and
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38 \bf Xavier Glorot \and
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39 Xavier Muller \and \\
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40 \bf Sylvain Pannetier Lebeuf \and
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41 Razvan Pascanu \and
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42 \bf Salah Rifai \and
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43 Francois Savard \and \\
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44 \bf Guillaume Sicard \\
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45 \vspace*{1mm}}
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46
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47 %I can't use aistatsaddress in a single side paragraphe.
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48 %The document is 2 colums, but this section span the 2 colums, sot there is only 1 left
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49 \center{Dept. IRO, U. Montreal, P.O. Box 6128, Centre-Ville branch, H3C 3J7, Montreal (Qc), Canada}
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50 \vspace*{5mm}
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51 ]
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52 %\aistatsaddress{Dept. IRO, U. Montreal, P.O. Box 6128, Centre-Ville branch, H3C 3J7, Montreal (Qc), Canada}
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53
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54
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55 %\vspace*{5mm}}
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56 %\date{{\tt bengioy@iro.umontreal.ca}, Dept. IRO, U. Montreal, P.O. Box 6128, Centre-Ville branch, H3C 3J7, Montreal (Qc), Canada}
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57 %\jmlrheading{}{2010}{}{10/2010}{XX/2011}{Yoshua Bengio et al}
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58 %\editor{}
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59
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60 %\makeanontitle
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61 %\maketitle
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62
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63 %{\bf Running title: Deep Self-Taught Learning}
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64
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65 \vspace*{5mm}
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66 \begin{abstract}
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67 Recent theoretical and empirical work in statistical machine learning has demonstrated the potential of learning algorithms for deep architectures, i.e., function classes obtained by composing multiple levels of representation. The hypothesis evaluated here is that intermediate levels of representation, because they can be shared across tasks and examples from different but related distributions, can yield even more benefits. Comparative experiments were performed on a large-scale handwritten character recognition setting with 62 classes (upper case, lower case, digits), using both a multi-task setting and perturbed examples in order to obtain out-of-distribution examples. The results agree with the hypothesis, and show that a deep learner did {\em beat previously published results and reached human-level performance}.
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68 \end{abstract}
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69 %\vspace*{-3mm}
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70
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71 %\begin{keywords}
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72 %Deep learning, self-taught learning, out-of-distribution examples, handwritten character recognition, multi-task learning
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73 %\end{keywords}
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74 %\keywords{self-taught learning \and multi-task learning \and out-of-distribution examples \and deep learning \and handwriting recognition}
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75
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76
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77
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78 \section{Introduction}
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79 %\vspace*{-1mm}
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80
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81 {\bf Deep Learning} has emerged as a promising new area of research in
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82 statistical machine learning~\citep{Hinton06,ranzato-07-small,Bengio-nips-2006,VincentPLarochelleH2008-very-small,ranzato-08,TaylorHintonICML2009,Larochelle-jmlr-2009,Salakhutdinov+Hinton-2009,HonglakL2009,HonglakLNIPS2009,Jarrett-ICCV2009,Taylor-cvpr-2010}. See \citet{Bengio-2009} for a review.
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83 Learning algorithms for deep architectures are centered on the learning
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84 of useful representations of data, which are better suited to the task at hand,
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85 and are organized in a hierarchy with multiple levels.
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86 This is in part inspired by observations of the mammalian visual cortex,
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87 which consists of a chain of processing elements, each of which is associated with a
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88 different representation of the raw visual input. In fact,
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89 it was found recently that the features learnt in deep architectures resemble
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90 those observed in the first two of these stages (in areas V1 and V2
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91 of visual cortex) \citep{HonglakL2008}, and that they become more and
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92 more invariant to factors of variation (such as camera movement) in
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93 higher layers~\citep{Goodfellow2009}.
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94 It has been hypothesized that learning a hierarchy of features increases the
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95 ease and practicality of developing representations that are at once
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96 tailored to specific tasks, yet are able to borrow statistical strength
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97 from other related tasks (e.g., modeling different kinds of objects). Finally, learning the
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98 feature representation can lead to higher-level (more abstract, more
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99 general) features that are more robust to unanticipated sources of
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100 variance extant in real data.
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101
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102 Whereas a deep architecture can in principle be more powerful than a
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103 shallow one in terms of representation, depth appears to render the
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104 training problem more difficult in terms of optimization and local minima.
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105 It is also only recently that successful algorithms were proposed to
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106 overcome some of these difficulties. All are based on unsupervised
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107 learning, often in an greedy layer-wise ``unsupervised pre-training''
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108 stage~\citep{Bengio-2009}.
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109 The principle is that each layer starting from
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110 the bottom is trained to represent its input (the output of the previous
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111 layer). After this
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112 unsupervised initialization, the stack of layers can be
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113 converted into a deep supervised feedforward neural network and fine-tuned by
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114 stochastic gradient descent.
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115 One of these layer initialization techniques,
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116 applied here, is the Denoising
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117 Auto-encoder~(DA)~\citep{VincentPLarochelleH2008-very-small} (see
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118 Figure~\ref{fig:da}), which performed similarly or
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119 better~\citep{VincentPLarochelleH2008-very-small} than previously
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120 proposed Restricted Boltzmann Machines (RBM)~\citep{Hinton06}
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121 in terms of unsupervised extraction
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122 of a hierarchy of features useful for classification. Each layer is trained
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123 to denoise its input, creating a layer of features that can be used as
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124 input for the next layer, forming a Stacked Denoising Auto-encoder (SDA).
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125 Note that training a Denoising Auto-encoder
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126 can actually been seen as training a particular RBM by an inductive
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127 principle different from maximum likelihood~\citep{Vincent-SM-2010},
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128 namely by Score Matching~\citep{Hyvarinen-2005,HyvarinenA2008}.
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129
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130 Previous comparative experimental results with stacking of RBMs and DAs
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131 to build deep supervised predictors had shown that they could outperform
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132 shallow architectures in a variety of settings, especially
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133 when the data involves complex interactions between many factors of
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134 variation~\citep{LarochelleH2007,Bengio-2009}. Other experiments have suggested
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135 that the unsupervised layer-wise pre-training acted as a useful
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136 prior~\citep{Erhan+al-2010} that allows one to initialize a deep
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137 neural network in a relatively much smaller region of parameter space,
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138 corresponding to better generalization.
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139
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140 To further the understanding of the reasons for the good performance
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141 observed with deep learners, we focus here on the following {\em hypothesis}:
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142 intermediate levels of representation, especially when there are
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143 more such levels, can be exploited to {\bf share
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144 statistical strength across different but related types of examples},
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145 such as examples coming from other tasks than the task of interest
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146 (the multi-task setting), or examples coming from an overlapping
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147 but different distribution (images with different kinds of perturbations
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148 and noises, here). This is consistent with the hypotheses discussed
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149 in~\citet{Bengio-2009} regarding the potential advantage
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150 of deep learning and the idea that more levels of representation can
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151 give rise to more abstract, more general features of the raw input.
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152
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153 This hypothesis is related to a learning setting called
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154 {\bf self-taught learning}~\citep{RainaR2007}, which combines principles
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155 of semi-supervised and multi-task learning: the learner can exploit examples
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156 that are unlabeled and possibly come from a distribution different from the target
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157 distribution, e.g., from other classes than those of interest.
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158 It has already been shown that deep learners can clearly take advantage of
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159 unsupervised learning and unlabeled examples~\citep{Bengio-2009,WestonJ2008-small},
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160 but more needed to be done to explore the impact
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161 of {\em out-of-distribution} examples and of the {\em multi-task} setting
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162 (one exception is~\citep{CollobertR2008}, which shares and uses unsupervised
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163 pre-training only with the first layer). In particular the {\em relative
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164 advantage of deep learning} for these settings has not been evaluated.
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165
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166
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167 %
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168 The {\bf main claim} of this paper is that deep learners (with several levels of representation) can
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169 {\bf benefit more from out-of-distribution examples than shallow learners} (with a single
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170 level), both in the context of the multi-task setting and from
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171 perturbed examples. Because we are able to improve on state-of-the-art
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172 performance and reach human-level performance
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173 on a large-scale task, we consider that this paper is also a contribution
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174 to advance the application of machine learning to handwritten character recognition.
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175 More precisely, we ask and answer the following questions:
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176
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177 %\begin{enumerate}
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178 $\bullet$ %\item
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179 Do the good results previously obtained with deep architectures on the
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180 MNIST digit images generalize to the setting of a similar but much larger and richer
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181 dataset, the NIST special database 19, with 62 classes and around 800k examples?
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182
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183 $\bullet$ %\item
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184 To what extent does the perturbation of input images (e.g. adding
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185 noise, affine transformations, background images) make the resulting
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186 classifiers better not only on similarly perturbed images but also on
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187 the {\em original clean examples}? We study this question in the
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188 context of the 62-class and 10-class tasks of the NIST special database 19.
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189
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190 $\bullet$ %\item
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191 Do deep architectures {\em benefit {\bf more} from such out-of-distribution}
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192 examples, in particular do they benefit more from
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193 examples that are perturbed versions of the examples from the task of interest?
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194
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195 $\bullet$ %\item
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196 Similarly, does the feature learning step in deep learning algorithms benefit {\bf more}
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197 from training with moderately {\em different classes} (i.e. a multi-task learning scenario) than
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198 a corresponding shallow and purely supervised architecture?
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199 We train on 62 classes and test on 10 (digits) or 26 (upper case or lower case)
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200 to answer this question.
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201 %\end{enumerate}
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202
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203 Our experimental results provide positive evidence towards all of these questions,
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204 as well as {\bf classifiers that reach human-level performance on 62-class isolated character
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205 recognition and beat previously published results on the NIST dataset (special database 19)}.
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206 To achieve these results, we introduce in the next section a sophisticated system
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207 for stochastically transforming character images and then explain the methodology,
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208 which is based on training with or without these transformed images and testing on
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209 clean ones.
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210 Code for generating these transformations as well as for the deep learning
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211 algorithms are made available at {\tt http://anonymous.url.net}.%{\tt http://hg.assembla.com/ift6266}.
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212
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213 %\vspace*{-3mm}
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214 %\newpage
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215 \section{Perturbed and Transformed Character Images}
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216 \label{s:perturbations}
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217 %\vspace*{-2mm}
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218
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219 Figure~\ref{fig:transform} shows the different transformations we used to stochastically
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220 transform $32 \times 32$ source images (such as the one in Fig.\ref{fig:torig})
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221 in order to obtain data from a larger distribution which
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222 covers a domain substantially larger than the clean characters distribution from
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223 which we start.
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224 Although character transformations have been used before to
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225 improve character recognizers, this effort is on a large scale both
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226 in number of classes and in the complexity of the transformations, hence
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227 in the complexity of the learning task.
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228 The code for these transformations (mostly Python) is available at
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229 {\tt http://anonymous.url.net}. All the modules in the pipeline (Figure~\ref{fig:transform}) share
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230 a global control parameter ($0 \le complexity \le 1$) that allows one to modulate the
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231 amount of deformation or noise introduced.
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232 There are two main parts in the pipeline. The first one,
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233 from thickness to pinch, performs transformations. The second
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234 part, from blur to contrast, adds different kinds of noise.
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235 More details can be found in~\citep{ift6266-tr-anonymous}.
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236
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237 \begin{figure*}[ht]
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238 \centering
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239 \subfigure[Original]{\includegraphics[scale=0.6]{images/Original.png}\label{fig:torig}}
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240 \subfigure[Thickness]{\includegraphics[scale=0.6]{images/Thick_only.png}}
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241 \subfigure[Slant]{\includegraphics[scale=0.6]{images/Slant_only.png}}
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242 \subfigure[Affine Transformation]{\includegraphics[scale=0.6]{images/Affine_only.png}}
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243 \subfigure[Local Elastic Deformation]{\includegraphics[scale=0.6]{images/Localelasticdistorsions_only.png}}
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244 \subfigure[Pinch]{\includegraphics[scale=0.6]{images/Pinch_only.png}}
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245 %Noise
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246 \subfigure[Motion Blur]{\includegraphics[scale=0.6]{images/Motionblur_only.png}}
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247 \subfigure[Occlusion]{\includegraphics[scale=0.6]{images/occlusion_only.png}}
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248 \subfigure[Gaussian Smoothing]{\includegraphics[scale=0.6]{images/Bruitgauss_only.png}}
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249 \subfigure[Pixels Permutation]{\includegraphics[scale=0.6]{images/Permutpixel_only.png}}
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250 \subfigure[Gaussian Noise]{\includegraphics[scale=0.6]{images/Distorsiongauss_only.png}}
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251 \subfigure[Background Image Addition]{\includegraphics[scale=0.6]{images/background_other_only.png}}
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252 \subfigure[Salt \& Pepper]{\includegraphics[scale=0.6]{images/Poivresel_only.png}}
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253 \subfigure[Scratches]{\includegraphics[scale=0.6]{images/Rature_only.png}}
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254 \subfigure[Grey Level \& Contrast]{\includegraphics[scale=0.6]{images/Contrast_only.png}}
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255 \caption{Top left (a): example original image. Others (b-o): examples of the effect
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256 of each transformation module taken separately. Actual perturbed examples are obtained by
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257 a pipeline of these, with random choices about which module to apply and how much perturbation
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258 to apply.}
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259 \label{fig:transform}
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260 %\vspace*{-2mm}
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261 \end{figure*}
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262
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263 %\vspace*{-3mm}
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264 \section{Experimental Setup}
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265 %\vspace*{-1mm}
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266
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267 Much previous work on deep learning had been performed on
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268 the MNIST digits task~\citep{Hinton06,ranzato-07-small,Bengio-nips-2006,Salakhutdinov+Hinton-2009},
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269 with 60,000 examples, and variants involving 10,000
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270 examples~\citep{Larochelle-jmlr-2009,VincentPLarochelleH2008-very-small}.
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271 The focus here is on much larger training sets, from 10 times to
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272 to 1000 times larger, and 62 classes.
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273
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274 The first step in constructing the larger datasets (called NISTP and P07) is to sample from
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275 a {\em data source}: {\bf NIST} (NIST database 19), {\bf Fonts}, {\bf Captchas},
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276 and {\bf OCR data} (scanned machine printed characters). See more in
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277 Section~\ref{sec:sources} below. Once a character
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278 is sampled from one of these sources (chosen randomly), the second step is to
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279 apply a pipeline of transformations and/or noise processes outlined in section \ref{s:perturbations}.
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280
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281 To provide a baseline of error rate comparison we also estimate human performance
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282 on both the 62-class task and the 10-class digits task.
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283 We compare the best Multi-Layer Perceptrons (MLP) against
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284 the best Stacked Denoising Auto-encoders (SDA), when
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285 both models' hyper-parameters are selected to minimize the validation set error.
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286 We also provide a comparison against a precise estimate
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287 of human performance obtained via Amazon's Mechanical Turk (AMT)
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288 service ({\tt http://mturk.com}).
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289 AMT users are paid small amounts
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290 of money to perform tasks for which human intelligence is required.
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291 Mechanical Turk has been used extensively in natural language processing and vision.
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292 %processing \citep{SnowEtAl2008} and vision
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293 %\citep{SorokinAndForsyth2008,whitehill09}.
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294 AMT users were presented
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295 with 10 character images (from a test set) on a screen
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296 and asked to label them.
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297 They were forced to choose a single character class (either among the
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298 62 or 10 character classes) for each image.
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299 80 subjects classified 2500 images per (dataset,task) pair.
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300 Different humans labelers sometimes provided a different label for the same
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301 example, and we were able to estimate the error variance due to this effect
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302 because each image was classified by 3 different persons.
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303 The average error of humans on the 62-class task NIST test set
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304 is 18.2\%, with a standard error of 0.1\%.
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305 We controlled noise in the labelling process by (1)
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306 requiring AMT workers with a higher than normal average of accepted
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307 responses ($>$95\%) on other tasks (2) discarding responses that were not
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308 complete (10 predictions) (3) discarding responses for which for which the
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309 time to predict was smaller than 3 seconds for NIST (the mean response time
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310 was 20 seconds) and 6 seconds seconds for NISTP (average response time of
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311 45 seconds) (4) discarding responses which were obviously wrong (10
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312 identical ones, or "12345..."). Overall, after such filtering, we kept
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313 approximately 95\% of the AMT workers' responses.
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314
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315 %\vspace*{-3mm}
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316 \subsection{Data Sources}
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317 \label{sec:sources}
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318 %\vspace*{-2mm}
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319
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320 %\begin{itemize}
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321 %\item
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322 {\bf NIST.}
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323 Our main source of characters is the NIST Special Database 19~\citep{Grother-1995},
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324 widely used for training and testing character
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325 recognition systems~\citep{Granger+al-2007,Cortes+al-2000,Oliveira+al-2002-short,Milgram+al-2005}.
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326 The dataset is composed of 814255 digits and characters (upper and lower cases), with hand checked classifications,
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327 extracted from handwritten sample forms of 3600 writers. The characters are labelled by one of the 62 classes
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328 corresponding to ``0''-``9'',``A''-``Z'' and ``a''-``z''. The dataset contains 8 parts (partitions) of varying complexity.
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329 The fourth partition (called $hsf_4$, 82,587 examples),
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330 experimentally recognized to be the most difficult one, is the one recommended
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331 by NIST as a testing set and is used in our work as well as some previous work~\citep{Granger+al-2007,Cortes+al-2000,Oliveira+al-2002-short,Milgram+al-2005}
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332 for that purpose. We randomly split the remainder (731,668 examples) into a training set and a validation set for
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333 model selection.
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334 The performances reported by previous work on that dataset mostly use only the digits.
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335 Here we use all the classes both in the training and testing phase. This is especially
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336 useful to estimate the effect of a multi-task setting.
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337 The distribution of the classes in the NIST training and test sets differs
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338 substantially, with relatively many more digits in the test set, and a more uniform distribution
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339 of letters in the test set (whereas in the training set they are distributed
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340 more like in natural text).
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341 %\vspace*{-1mm}
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342
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343 %\item
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344 {\bf Fonts.}
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345 In order to have a good variety of sources we downloaded an important number of free fonts from:
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346 {\tt http://cg.scs.carleton.ca/\textasciitilde luc/freefonts.html}.
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347 % TODO: pointless to anonymize, it's not pointing to our work
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348 Including an operating system's (Windows 7) fonts, there is a total of $9817$ different fonts that we can choose uniformly from.
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349 The chosen {\tt ttf} file is either used as input of the Captcha generator (see next item) or, by producing a corresponding image,
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350 directly as input to our models.
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351 %\vspace*{-1mm}
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352
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353 %\item
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354 {\bf Captchas.}
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355 The Captcha data source is an adaptation of the \emph{pycaptcha} library (a Python-based captcha generator library) for
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356 generating characters of the same format as the NIST dataset. This software is based on
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357 a random character class generator and various kinds of transformations similar to those described in the previous sections.
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358 In order to increase the variability of the data generated, many different fonts are used for generating the characters.
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359 Transformations (slant, distortions, rotation, translation) are applied to each randomly generated character with a complexity
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360 depending on the value of the complexity parameter provided by the user of the data source.
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361 %Two levels of complexity are allowed and can be controlled via an easy to use facade class. %TODO: what's a facade class?
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362 %\vspace*{-1mm}
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363
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364 %\item
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365 {\bf OCR data.}
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366 A large set (2 million) of scanned, OCRed and manually verified machine-printed
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367 characters where included as an
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368 additional source. This set is part of a larger corpus being collected by the Image Understanding
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369 Pattern Recognition Research group led by Thomas Breuel at University of Kaiserslautern
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370 ({\tt http://www.iupr.com}), and which will be publicly released.
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371 %TODO: let's hope that Thomas is not a reviewer! :) Seriously though, maybe we should anonymize this
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372 %\end{itemize}
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373
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374 %\vspace*{-3mm}
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375 \subsection{Data Sets}
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376 %\vspace*{-2mm}
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377
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378 All data sets contain 32$\times$32 grey-level images (values in $[0,1]$) associated with a label
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379 from one of the 62 character classes.
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380 %\begin{itemize}
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381 %\vspace*{-1mm}
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382
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383 %\item
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384 {\bf NIST.} This is the raw NIST special database 19~\citep{Grother-1995}. It has
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385 \{651,668 / 80,000 / 82,587\} \{training / validation / test\} examples.
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386 %\vspace*{-1mm}
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387
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388 %\item
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389 {\bf P07.} This dataset is obtained by taking raw characters from all four of the above sources
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390 and sending them through the transformation pipeline described in section \ref{s:perturbations}.
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391 For each new example to generate, a data source is selected with probability $10\%$ from the fonts,
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392 $25\%$ from the captchas, $25\%$ from the OCR data and $40\%$ from NIST. We apply all the transformations in the
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393 order given above, and for each of them we sample uniformly a \emph{complexity} in the range $[0,0.7]$.
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394 It has \{81,920,000 / 80,000 / 20,000\} \{training / validation / test\} examples
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395 obtained from the corresponding NIST sets plus other sources.
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396 %\vspace*{-1mm}
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397
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398 %\item
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399 {\bf NISTP.} This one is equivalent to P07 (complexity parameter of $0.7$ with the same proportions of data sources)
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400 except that we only apply
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401 transformations from slant to pinch (see Fig.\ref{fig:transform}(b-f)).
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402 Therefore, the character is
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403 transformed but no additional noise is added to the image, giving images
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404 closer to the NIST dataset.
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405 It has \{81,920,000 / 80,000 / 20,000\} \{training / validation / test\} examples
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406 obtained from the corresponding NIST sets plus other sources.
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407 %\end{itemize}
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408
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409 \begin{figure*}[ht]
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410 %\vspace*{-2mm}
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411 \centerline{\resizebox{0.8\textwidth}{!}{\includegraphics{images/denoising_autoencoder_small.pdf}}}
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412 %\vspace*{-2mm}
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413 \caption{Illustration of the computations and training criterion for the denoising
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414 auto-encoder used to pre-train each layer of the deep architecture. Input $x$ of
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415 the layer (i.e. raw input or output of previous layer)
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416 s corrupted into $\tilde{x}$ and encoded into code $y$ by the encoder $f_\theta(\cdot)$.
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417 The decoder $g_{\theta'}(\cdot)$ maps $y$ to reconstruction $z$, which
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418 is compared to the uncorrupted input $x$ through the loss function
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419 $L_H(x,z)$, whose expected value is approximately minimized during training
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420 by tuning $\theta$ and $\theta'$.}
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421 \label{fig:da}
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422 %\vspace*{-2mm}
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423 \end{figure*}
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424
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425 %\vspace*{-3mm}
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426 \subsection{Models and their Hyper-parameters}
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427 %\vspace*{-2mm}
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428
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429 The experiments are performed using MLPs (with a single
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430 hidden layer) and deep SDAs.
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431 \emph{Hyper-parameters are selected based on the {\bf NISTP} validation set error.}
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432
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433 {\bf Multi-Layer Perceptrons (MLP).} The MLP output estimated
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434 \[
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435 P({\rm class}|{\rm input}=x)
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436 \]
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437 with
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438 \[
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439 f(x)={\rm softmax}(b_2+W_2\tanh(b_1+W_1 x)),
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440 \]
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441 i.e., two layers, where
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442 \[
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443 p={\rm softmax}(a)
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444 \]
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445 means that
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446 \[
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447 p_i(x)=\exp(a_i)/\sum_j \exp(a_j)
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448 \]
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449 representing the probability
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450 for class $i$, $\tanh$ is the element-wise
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451 hyperbolic tangent, $b_i$ are parameter vectors, and $W_i$ are
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452 parameter matrices (one per layer). The
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453 number of rows of $W_1$ is called the number of hidden units (of the
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454 single hidden layer, here), and
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455 is one way to control capacity (the main other ways to control capacity are
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456 the number of training iterations and optionally a regularization penalty
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457 on the parameters, not used here because it did not help).
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458 Whereas previous work had compared
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459 deep architectures to both shallow MLPs and SVMs, we only compared to MLPs
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460 here because of the very large datasets used (making the use of SVMs
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461 computationally challenging because of their quadratic scaling
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462 behavior). Preliminary experiments on training SVMs (libSVM) with subsets
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463 of the training set allowing the program to fit in memory yielded
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464 substantially worse results than those obtained with MLPs\footnote{RBF SVMs
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465 trained with a subset of NISTP or NIST, 100k examples, to fit in memory,
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466 yielded 64\% test error or worse; online linear SVMs trained on the whole
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467 of NIST or 800k from NISTP yielded no better than 42\% error; slightly
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468 better results were obtained by sparsifying the pixel intensities and
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469 projecting to a second-order polynomial (a very sparse vector), still
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470 41\% error. We expect that better results could be obtained with a
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471 better implementation allowing for training with more examples and
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472 a higher-order non-linear projection.} For training on nearly a hundred million examples (with the
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473 perturbed data), the MLPs and SDA are much more convenient than classifiers
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474 based on kernel methods. The MLP has a single hidden layer with $\tanh$
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475 activation functions, and softmax (normalized exponentials) on the output
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476 layer for estimating $P({\rm class} | {\rm input})$. The number of hidden units is
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477 taken in $\{300,500,800,1000,1500\}$. Training examples are presented in
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478 minibatches of size 20, i.e., the parameters are iteratively updated in the direction
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479 of the mean gradient of the next 20 examples. A constant learning rate was chosen among $\{0.001,
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480 0.01, 0.025, 0.075, 0.1, 0.5\}$.
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481 %through preliminary experiments (measuring performance on a validation set),
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482 %and $0.1$ (which was found to work best) was then selected for optimizing on
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483 %the whole training sets.
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484 %\vspace*{-1mm}
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485
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486
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487 {\bf Stacked Denoising Auto-encoders (SDA).}
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488 Various auto-encoder variants and Restricted Boltzmann Machines (RBMs)
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489 can be used to initialize the weights of each layer of a deep MLP (with many hidden
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490 layers)~\citep{Hinton06,ranzato-07-small,Bengio-nips-2006},
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491 apparently setting parameters in the
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492 basin of attraction of supervised gradient descent yielding better
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493 generalization~\citep{Erhan+al-2010}. This initial {\em unsupervised
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494 pre-training phase} uses all of the training images but not the training labels.
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495 Each layer is trained in turn to produce a new representation of its input
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496 (starting from the raw pixels).
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497 It is hypothesized that the
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498 advantage brought by this procedure stems from a better prior,
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499 on the one hand taking advantage of the link between the input
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500 distribution $P(x)$ and the conditional distribution of interest
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501 $P(y|x)$ (like in semi-supervised learning), and on the other hand
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502 taking advantage of the expressive power and bias implicit in the
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503 deep architecture (whereby complex concepts are expressed as
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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504 compositions of simpler ones through a deep hierarchy).
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505
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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506 Here we chose to use the Denoising
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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507 Auto-encoder~\citep{VincentPLarochelleH2008-very-small} as the building block for
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508 these deep hierarchies of features, as it is simple to train and
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509 explain (see Figure~\ref{fig:da}, as well as
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510 tutorial and code there: {\tt http://deeplearning.net/tutorial}),
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511 provides efficient inference, and yielded results
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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512 comparable or better than RBMs in series of experiments
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513 \citep{VincentPLarochelleH2008-very-small}. It really corresponds to a Gaussian
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514 RBM trained by a Score Matching criterion~\cite{Vincent-SM-2010}.
631
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515 During its unsupervised training, a Denoising
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516 Auto-encoder is presented with a stochastically corrupted version $\tilde{x}$
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517 of the input $x$ and trained to reconstruct to produce a reconstruction $z$
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diff changeset
518 of the uncorrupted input $x$. Because the network has to denoise, it is
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diff changeset
519 forcing the hidden units $y$ to represent the leading regularities in
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diff changeset
520 the data. Following~\citep{VincentPLarochelleH2008-very-small}
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diff changeset
521 the hidden units output $y$ is obtained through
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diff changeset
522 \[
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523 y={\rm sigm}(c+V x)
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diff changeset
524 \]
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diff changeset
525 where ${\rm sigm}(a)=1/(1+\exp(-a))$
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diff changeset
526 and the reconstruction is
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527 \[
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528 z={\rm sigm}(d+V' y).
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529 \]
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530 We minimize the training
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531 set average of the cross-entropy
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532 reconstruction error
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533 \[
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534 L_H(x,z)=\sum_i z_i \log x_i + (1-z_i) \log(1-x_i).
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535 \]
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diff changeset
536 Here we use the random binary masking corruption
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537 (which in $\tilde{x}$ sets to 0 a random subset of the elements of $x$, and
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diff changeset
538 copies the rest).
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diff changeset
539 Once the first denoising auto-encoder is trained, its parameters can be used
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540 to set the first layer of the deep MLP. The original data are then processed
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541 through that first layer, and the output of the hidden units form a new
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diff changeset
542 representation that can be used as input data for training a second denoising
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543 auto-encoder, still in a purely unsupervised way.
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diff changeset
544 This is repeated for the desired number of hidden layers.
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545 After this unsupervised pre-training stage, the parameters
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diff changeset
546 are used to initialize a deep MLP (similar to the above, but
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547 with more layers), which is fine-tuned by
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diff changeset
548 the same standard procedure (stochastic gradient descent)
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549 used to train MLPs in general (see above).
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diff changeset
550 The top layer parameters of the deep MLP (the one which outputs the
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diff changeset
551 class probabilities and takes the top hidden layer as input) can
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552 be initialized at 0.
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553 The SDA hyper-parameters are the same as for the MLP, with the addition of the
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554 amount of corruption noise (we used the masking noise process, whereby a
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555 fixed proportion of the input values, randomly selected, are zeroed), and a
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556 separate learning rate for the unsupervised pre-training stage (selected
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
557 from the same above set). The fraction of inputs corrupted was selected
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
558 among $\{10\%, 20\%, 50\%\}$. Another hyper-parameter is the number
631
510220effb14 corrections demandees par reviewer
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 630
diff changeset
559 of hidden layers but it was fixed to 3 for our experiments,
627
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
560 based on previous work with
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
561 SDAs on MNIST~\citep{VincentPLarochelleH2008-very-small}.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
562 We also compared against 1 and against 2 hidden layers, in order
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
563 to disantangle the effect of depth from the effect of unsupervised
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
564 pre-training.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
565 The size of the hidden
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
566 layers was kept constant across hidden layers, and the best results
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
567 were obtained with the largest values that we could experiment
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
568 with given our patience, with 1000 hidden units.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
569
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
570 %\vspace*{-1mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
571
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
572 \begin{figure*}[ht]
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
573 %\vspace*{-2mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
574 \centerline{\resizebox{.99\textwidth}{!}{\includegraphics{images/error_rates_charts.pdf}}}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
575 %\vspace*{-3mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
576 \caption{SDAx are the {\bf deep} models. Error bars indicate a 95\% confidence interval. 0 indicates that the model was trained
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
577 on NIST, 1 on NISTP, and 2 on P07. Left: overall results
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
578 of all models, on NIST and NISTP test sets.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
579 Right: error rates on NIST test digits only, along with the previous results from
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
580 literature~\citep{Granger+al-2007,Cortes+al-2000,Oliveira+al-2002-short,Milgram+al-2005}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
581 respectively based on ART, nearest neighbors, MLPs, and SVMs.}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
582 \label{fig:error-rates-charts}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
583 %\vspace*{-2mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
584 \end{figure*}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
585
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
586
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
587 \begin{figure*}[ht]
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
588 \vspace*{-3mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
589 \centerline{\resizebox{.99\textwidth}{!}{\includegraphics{images/improvements_charts.pdf}}}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
590 \vspace*{-3mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
591 \caption{Relative improvement in error rate due to out-of-distribution examples.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
592 Left: Improvement (or loss, when negative)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
593 induced by out-of-distribution examples (perturbed data).
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
594 Right: Improvement (or loss, when negative) induced by multi-task
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
595 learning (training on all classes and testing only on either digits,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
596 upper case, or lower-case). The deep learner (SDA) benefits more from
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
597 out-of-distribution examples, compared to the shallow MLP.}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
598 \label{fig:improvements-charts}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
599 \vspace*{-2mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
600 \end{figure*}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
601
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
602 \vspace*{-2mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
603 \section{Experimental Results}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
604 \vspace*{-2mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
605
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
606 %%\vspace*{-1mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
607 %\subsection{SDA vs MLP vs Humans}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
608 %%\vspace*{-1mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
609 The models are either trained on NIST (MLP0 and SDA0),
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
610 NISTP (MLP1 and SDA1), or P07 (MLP2 and SDA2), and tested
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
611 on either NIST, NISTP or P07 (regardless of the data set used for training),
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
612 either on the 62-class task
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
613 or on the 10-digits task. Training time (including about half
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
614 for unsupervised pre-training, for DAs) on the larger
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
615 datasets is around one day on a GPU (GTX 285).
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
616 Figure~\ref{fig:error-rates-charts} summarizes the results obtained,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
617 comparing humans, the three MLPs (MLP0, MLP1, MLP2) and the three SDAs (SDA0, SDA1,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
618 SDA2), along with the previous results on the digits NIST special database
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
619 19 test set from the literature, respectively based on ARTMAP neural
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
620 networks ~\citep{Granger+al-2007}, fast nearest-neighbor search
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
621 ~\citep{Cortes+al-2000}, MLPs ~\citep{Oliveira+al-2002-short}, and SVMs
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
622 ~\citep{Milgram+al-2005}.% More detailed and complete numerical results
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
623 %(figures and tables, including standard errors on the error rates) can be
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
624 %found in Appendix.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
625 The deep learner not only outperformed the shallow ones and
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
626 previously published performance (in a statistically and qualitatively
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
627 significant way) but when trained with perturbed data
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
628 reaches human performance on both the 62-class task
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
629 and the 10-class (digits) task.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
630 17\% error (SDA1) or 18\% error (humans) may seem large but a large
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
631 majority of the errors from humans and from SDA1 are from out-of-context
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
632 confusions (e.g. a vertical bar can be a ``1'', an ``l'' or an ``L'', and a
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
633 ``c'' and a ``C'' are often indistinguishible).
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
634 Regarding shallower networks pre-trained with unsupervised denoising
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
635 auto-encders, we find that the NIST test error is 21\% with one hidden
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
636 layer and 20\% with two hidden layers (vs 17\% in the same conditions
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
637 with 3 hidden layers). Compare this with the 23\% error achieved
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
638 by the MLP, i.e. a single hidden layer and no unsupervised pre-training.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
639 As found in previous work~\cite{Erhan+al-2010,Larochelle-jmlr-2009},
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
640 these results show that both depth and
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
641 unsupervised pre-training need to be combined in order to achieve
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
642 the best results.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
643
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
644
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
645 In addition, as shown in the left of
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
646 Figure~\ref{fig:improvements-charts}, the relative improvement in error
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
647 rate brought by out-of-distribution examples is greater for the deep
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
648 SDA, and these
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
649 differences with the shallow MLP are statistically and qualitatively
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
650 significant.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
651 The left side of the figure shows the improvement to the clean
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
652 NIST test set error brought by the use of out-of-distribution examples
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
653 (i.e. the perturbed examples examples from NISTP or P07),
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
654 over the models trained exclusively on NIST (respectively SDA0 and MLP0).
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
655 Relative percent change is measured by taking
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
656 $100 \% \times$ (original model's error / perturbed-data model's error - 1).
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
657 The right side of
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
658 Figure~\ref{fig:improvements-charts} shows the relative improvement
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
659 brought by the use of a multi-task setting, in which the same model is
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
660 trained for more classes than the target classes of interest (i.e. training
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
661 with all 62 classes when the target classes are respectively the digits,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
662 lower-case, or upper-case characters). Again, whereas the gain from the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
663 multi-task setting is marginal or negative for the MLP, it is substantial
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
664 for the SDA. Note that to simplify these multi-task experiments, only the original
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
665 NIST dataset is used. For example, the MLP-digits bar shows the relative
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
666 percent improvement in MLP error rate on the NIST digits test set
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
667 as $100\% \times$ (single-task
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
668 model's error / multi-task model's error - 1). The single-task model is
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
669 trained with only 10 outputs (one per digit), seeing only digit examples,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
670 whereas the multi-task model is trained with 62 outputs, with all 62
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
671 character classes as examples. Hence the hidden units are shared across
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
672 all tasks. For the multi-task model, the digit error rate is measured by
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
673 comparing the correct digit class with the output class associated with the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
674 maximum conditional probability among only the digit classes outputs. The
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
675 setting is similar for the other two target classes (lower case characters
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
676 and upper case characters). Note however that some types of perturbations
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
677 (NISTP) help more than others (P07) when testing on the clean images.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
678 %%\vspace*{-1mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
679 %\subsection{Perturbed Training Data More Helpful for SDA}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
680 %%\vspace*{-1mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
681
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
682 %%\vspace*{-1mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
683 %\subsection{Multi-Task Learning Effects}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
684 %%\vspace*{-1mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
685
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
686 \iffalse
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
687 As previously seen, the SDA is better able to benefit from the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
688 transformations applied to the data than the MLP. In this experiment we
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
689 define three tasks: recognizing digits (knowing that the input is a digit),
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
690 recognizing upper case characters (knowing that the input is one), and
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
691 recognizing lower case characters (knowing that the input is one). We
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
692 consider the digit classification task as the target task and we want to
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
693 evaluate whether training with the other tasks can help or hurt, and
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
694 whether the effect is different for MLPs versus SDAs. The goal is to find
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
695 out if deep learning can benefit more (or less) from multiple related tasks
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
696 (i.e. the multi-task setting) compared to a corresponding purely supervised
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
697 shallow learner.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
698
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
699 We use a single hidden layer MLP with 1000 hidden units, and a SDA
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
700 with 3 hidden layers (1000 hidden units per layer), pre-trained and
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
701 fine-tuned on NIST.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
702
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
703 Our results show that the MLP benefits marginally from the multi-task setting
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
704 in the case of digits (5\% relative improvement) but is actually hurt in the case
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
705 of characters (respectively 3\% and 4\% worse for lower and upper class characters).
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
706 On the other hand the SDA benefited from the multi-task setting, with relative
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
707 error rate improvements of 27\%, 15\% and 13\% respectively for digits,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
708 lower and upper case characters, as shown in Table~\ref{tab:multi-task}.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
709 \fi
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
710
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
711
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
712 \vspace*{-2mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
713 \section{Conclusions and Discussion}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
714 \vspace*{-2mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
715
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
716 We have found that out-of-distribution examples (multi-task learning
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
717 and perturbed examples) are more beneficial
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
718 to a deep learner than to a traditional shallow and purely
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
719 supervised learner. More precisely,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
720 the answers are positive for all the questions asked in the introduction.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
721 %\begin{itemize}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
722
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
723 $\bullet$ %\item
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
724 {\bf Do the good results previously obtained with deep architectures on the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
725 MNIST digits generalize to a much larger and richer (but similar)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
726 dataset, the NIST special database 19, with 62 classes and around 800k examples}?
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
727 Yes, the SDA {\em systematically outperformed the MLP and all the previously
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
728 published results on this dataset} (the ones that we are aware of), {\em in fact reaching human-level
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
729 performance} at around 17\% error on the 62-class task and 1.4\% on the digits,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
730 and beating previously published results on the same data.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
731
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
732 $\bullet$ %\item
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
733 {\bf To what extent do out-of-distribution examples help deep learners,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
734 and do they help them more than shallow supervised ones}?
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
735 We found that distorted training examples not only made the resulting
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
736 classifier better on similarly perturbed images but also on
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
737 the {\em original clean examples}, and more importantly and more novel,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
738 that deep architectures benefit more from such {\em out-of-distribution}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
739 examples. Shallow MLPs were helped by perturbed training examples when tested on perturbed input
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
740 images (65\% relative improvement on NISTP)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
741 but only marginally helped (5\% relative improvement on all classes)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
742 or even hurt (10\% relative loss on digits)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
743 with respect to clean examples. On the other hand, the deep SDAs
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
744 were significantly boosted by these out-of-distribution examples.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
745 Similarly, whereas the improvement due to the multi-task setting was marginal or
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
746 negative for the MLP (from +5.6\% to -3.6\% relative change),
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
747 it was quite significant for the SDA (from +13\% to +27\% relative change),
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
748 which may be explained by the arguments below.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
749 Since out-of-distribution data
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
750 (perturbed or from other related classes) is very common, this conclusion
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
751 is of practical importance.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
752 %\end{itemize}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
753
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
754 In the original self-taught learning framework~\citep{RainaR2007}, the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
755 out-of-sample examples were used as a source of unsupervised data, and
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
756 experiments showed its positive effects in a \emph{limited labeled data}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
757 scenario. However, many of the results by \citet{RainaR2007} (who used a
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
758 shallow, sparse coding approach) suggest that the {\em relative gain of self-taught
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
759 learning vs ordinary supervised learning} diminishes as the number of labeled examples increases.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
760 We note instead that, for deep
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
761 architectures, our experiments show that such a positive effect is accomplished
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
762 even in a scenario with a \emph{large number of labeled examples},
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
763 i.e., here, the relative gain of self-taught learning and
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
764 out-of-distribution examples is probably preserved
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
765 in the asymptotic regime. However, note that in our perturbation experiments
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
766 (but not in our multi-task experiments),
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
767 even the out-of-distribution examples are labeled, unlike in the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
768 earlier self-taught learning experiments~\citep{RainaR2007}.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
769
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
770 {\bf Why would deep learners benefit more from the self-taught learning
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
771 framework and out-of-distribution examples}?
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
772 The key idea is that the lower layers of the predictor compute a hierarchy
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
773 of features that can be shared across tasks or across variants of the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
774 input distribution. A theoretical analysis of generalization improvements
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
775 due to sharing of intermediate features across tasks already points
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
776 towards that explanation~\cite{baxter95a}.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
777 Intermediate features that can be used in different
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
778 contexts can be estimated in a way that allows to share statistical
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
779 strength. Features extracted through many levels are more likely to
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
780 be more abstract and more invariant to some of the factors of variation
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
781 in the underlying distribution (as the experiments in~\citet{Goodfellow2009} suggest),
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
782 increasing the likelihood that they would be useful for a larger array
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
783 of tasks and input conditions.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
784 Therefore, we hypothesize that both depth and unsupervised
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
785 pre-training play a part in explaining the advantages observed here, and future
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
786 experiments could attempt at teasing apart these factors.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
787 And why would deep learners benefit from the self-taught learning
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
788 scenarios even when the number of labeled examples is very large?
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
789 We hypothesize that this is related to the hypotheses studied
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
790 in~\citet{Erhan+al-2010}. In~\citet{Erhan+al-2010}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
791 it was found that online learning on a huge dataset did not make the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
792 advantage of the deep learning bias vanish, and a similar phenomenon
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
793 may be happening here. We hypothesize that unsupervised pre-training
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
794 of a deep hierarchy with out-of-distribution examples initializes the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
795 model in the basin of attraction of supervised gradient descent
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
796 that corresponds to better generalization. Furthermore, such good
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
797 basins of attraction are not discovered by pure supervised learning
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
798 (with or without out-of-distribution examples) from random initialization, and more labeled examples
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
799 does not allow the shallow or purely supervised models to discover
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
800 the kind of better basins associated
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
801 with deep learning and out-of-distribution examples.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
802
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
803 A Flash demo of the recognizer (where both the MLP and the SDA can be compared)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
804 can be executed on-line at the anonymous site {\tt http://deep.host22.com}.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
805
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
806 \iffalse
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
807 \section*{Appendix I: Detailed Numerical Results}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
808
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
809 These tables correspond to Figures 2 and 3 and contain the raw error rates for each model and dataset considered.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
810 They also contain additional data such as test errors on P07 and standard errors.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
811
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
812 \begin{table}[ht]
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
813 \caption{Overall comparison of error rates ($\pm$ std.err.) on 62 character classes (10 digits +
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
814 26 lower + 26 upper), except for last columns -- digits only, between deep architecture with pre-training
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
815 (SDA=Stacked Denoising Autoencoder) and ordinary shallow architecture
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
816 (MLP=Multi-Layer Perceptron). The models shown are all trained using perturbed data (NISTP or P07)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
817 and using a validation set to select hyper-parameters and other training choices.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
818 \{SDA,MLP\}0 are trained on NIST,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
819 \{SDA,MLP\}1 are trained on NISTP, and \{SDA,MLP\}2 are trained on P07.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
820 The human error rate on digits is a lower bound because it does not count digits that were
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
821 recognized as letters. For comparison, the results found in the literature
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
822 on NIST digits classification using the same test set are included.}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
823 \label{tab:sda-vs-mlp-vs-humans}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
824 \begin{center}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
825 \begin{tabular}{|l|r|r|r|r|} \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
826 & NIST test & NISTP test & P07 test & NIST test digits \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
827 Humans& 18.2\% $\pm$.1\% & 39.4\%$\pm$.1\% & 46.9\%$\pm$.1\% & $1.4\%$ \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
828 SDA0 & 23.7\% $\pm$.14\% & 65.2\%$\pm$.34\% & 97.45\%$\pm$.06\% & 2.7\% $\pm$.14\%\\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
829 SDA1 & 17.1\% $\pm$.13\% & 29.7\%$\pm$.3\% & 29.7\%$\pm$.3\% & 1.4\% $\pm$.1\%\\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
830 SDA2 & 18.7\% $\pm$.13\% & 33.6\%$\pm$.3\% & 39.9\%$\pm$.17\% & 1.7\% $\pm$.1\%\\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
831 MLP0 & 24.2\% $\pm$.15\% & 68.8\%$\pm$.33\% & 78.70\%$\pm$.14\% & 3.45\% $\pm$.15\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
832 MLP1 & 23.0\% $\pm$.15\% & 41.8\%$\pm$.35\% & 90.4\%$\pm$.1\% & 3.85\% $\pm$.16\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
833 MLP2 & 24.3\% $\pm$.15\% & 46.0\%$\pm$.35\% & 54.7\%$\pm$.17\% & 4.85\% $\pm$.18\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
834 \citep{Granger+al-2007} & & & & 4.95\% $\pm$.18\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
835 \citep{Cortes+al-2000} & & & & 3.71\% $\pm$.16\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
836 \citep{Oliveira+al-2002} & & & & 2.4\% $\pm$.13\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
837 \citep{Milgram+al-2005} & & & & 2.1\% $\pm$.12\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
838 \end{tabular}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
839 \end{center}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
840 \end{table}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
841
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
842 \begin{table}[ht]
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
843 \caption{Relative change in error rates due to the use of perturbed training data,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
844 either using NISTP, for the MLP1/SDA1 models, or using P07, for the MLP2/SDA2 models.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
845 A positive value indicates that training on the perturbed data helped for the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
846 given test set (the first 3 columns on the 62-class tasks and the last one is
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
847 on the clean 10-class digits). Clearly, the deep learning models did benefit more
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
848 from perturbed training data, even when testing on clean data, whereas the MLP
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
849 trained on perturbed data performed worse on the clean digits and about the same
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
850 on the clean characters. }
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
851 \label{tab:perturbation-effect}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
852 \begin{center}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
853 \begin{tabular}{|l|r|r|r|r|} \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
854 & NIST test & NISTP test & P07 test & NIST test digits \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
855 SDA0/SDA1-1 & 38\% & 84\% & 228\% & 93\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
856 SDA0/SDA2-1 & 27\% & 94\% & 144\% & 59\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
857 MLP0/MLP1-1 & 5.2\% & 65\% & -13\% & -10\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
858 MLP0/MLP2-1 & -0.4\% & 49\% & 44\% & -29\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
859 \end{tabular}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
860 \end{center}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
861 \end{table}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
862
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
863 \begin{table}[ht]
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
864 \caption{Test error rates and relative change in error rates due to the use of
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
865 a multi-task setting, i.e., training on each task in isolation vs training
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
866 for all three tasks together, for MLPs vs SDAs. The SDA benefits much
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
867 more from the multi-task setting. All experiments on only on the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
868 unperturbed NIST data, using validation error for model selection.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
869 Relative improvement is 1 - single-task error / multi-task error.}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
870 \label{tab:multi-task}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
871 \begin{center}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
872 \begin{tabular}{|l|r|r|r|} \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
873 & single-task & multi-task & relative \\
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
874 & setting & setting & improvement \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
875 MLP-digits & 3.77\% & 3.99\% & 5.6\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
876 MLP-lower & 17.4\% & 16.8\% & -4.1\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
877 MLP-upper & 7.84\% & 7.54\% & -3.6\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
878 SDA-digits & 2.6\% & 3.56\% & 27\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
879 SDA-lower & 12.3\% & 14.4\% & 15\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
880 SDA-upper & 5.93\% & 6.78\% & 13\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
881 \end{tabular}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
882 \end{center}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
883 \end{table}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
884
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
885 \fi
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
886
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
887 %\afterpage{\clearpage}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
888 %\clearpage
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
889 {
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
890 %\bibliographystyle{spbasic} % basic style, author-year citations
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
891 \bibliographystyle{plainnat}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
892 \bibliography{strings,strings-short,strings-shorter,ift6266_ml,specials,aigaion-shorter}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
893 %\bibliographystyle{unsrtnat}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
894 %\bibliographystyle{apalike}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
895 }
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
896
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
897
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
898 \end{document}