annotate writeup/aistats2011_cameraready.tex @ 638:677d1b1d8158

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author Yoshua Bengio <bengioy@iro.umontreal.ca>
date Sat, 19 Mar 2011 23:11:17 -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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20
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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
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212 {\tt http://hg.assembla.com/ift6266}.
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213
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214 %\vspace*{-3mm}
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215 %\newpage
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216 \section{Perturbed and Transformed Character Images}
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217 \label{s:perturbations}
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218 %\vspace*{-2mm}
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219
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220 Figure~\ref{fig:transform} shows the different transformations we used to stochastically
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221 transform $32 \times 32$ source images (such as the one in Fig.\ref{fig:torig})
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222 in order to obtain data from a larger distribution which
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223 covers a domain substantially larger than the clean characters distribution from
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224 which we start.
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225 Although character transformations have been used before to
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226 improve character recognizers, this effort is on a large scale both
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227 in number of classes and in the complexity of the transformations, hence
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228 in the complexity of the learning task.
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229 The code for these transformations (mostly Python) is available at
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230 {\tt http://hg.assembla.com/ift6266}. All the modules in the pipeline (Figure~\ref{fig:transform}) share
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231 a global control parameter ($0 \le complexity \le 1$) that allows one to modulate the
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232 amount of deformation or noise introduced.
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233 There are two main parts in the pipeline. The first one,
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234 from thickness to pinch, performs transformations. The second
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235 part, from blur to contrast, adds different kinds of noise.
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236 More details can be found in~\citep{ARXIV-2010}.
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237
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238 \begin{figure*}[ht]
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239 \centering
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240 \subfigure[Original]{\includegraphics[scale=0.6]{images/Original.png}\label{fig:torig}}
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241 \subfigure[Thickness]{\includegraphics[scale=0.6]{images/Thick_only.png}}
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242 \subfigure[Slant]{\includegraphics[scale=0.6]{images/Slant_only.png}}
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243 \subfigure[Affine Transformation]{\includegraphics[scale=0.6]{images/Affine_only.png}}
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244 \subfigure[Local Elastic Deformation]{\includegraphics[scale=0.6]{images/Localelasticdistorsions_only.png}}
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245 \subfigure[Pinch]{\includegraphics[scale=0.6]{images/Pinch_only.png}}
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246 %Noise
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247 \subfigure[Motion Blur]{\includegraphics[scale=0.6]{images/Motionblur_only.png}}
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248 \subfigure[Occlusion]{\includegraphics[scale=0.6]{images/occlusion_only.png}}
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249 \subfigure[Gaussian Smoothing]{\includegraphics[scale=0.6]{images/Bruitgauss_only.png}}
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250 \subfigure[Pixels Permutation]{\includegraphics[scale=0.6]{images/Permutpixel_only.png}}
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251 \subfigure[Gaussian Noise]{\includegraphics[scale=0.6]{images/Distorsiongauss_only.png}}
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252 \subfigure[Background Image Addition]{\includegraphics[scale=0.6]{images/background_other_only.png}}
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253 \subfigure[Salt \& Pepper]{\includegraphics[scale=0.6]{images/Poivresel_only.png}}
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254 \subfigure[Scratches]{\includegraphics[scale=0.6]{images/Rature_only.png}}
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255 \subfigure[Grey Level \& Contrast]{\includegraphics[scale=0.6]{images/Contrast_only.png}}
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256 \caption{Top left (a): example original image. Others (b-o): examples of the effect
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257 of each transformation module taken separately. Actual perturbed examples are obtained by
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258 a pipeline of these, with random choices about which module to apply and how much perturbation
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259 to apply.}
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260 \label{fig:transform}
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261 %\vspace*{-2mm}
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262 \end{figure*}
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263
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264 %\vspace*{-3mm}
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265 \section{Experimental Setup}
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266 %\vspace*{-1mm}
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267
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268 Much previous work on deep learning had been performed on
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269 the MNIST digits task~\citep{Hinton06,ranzato-07-small,Bengio-nips-2006,Salakhutdinov+Hinton-2009},
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270 with 60,000 examples, and variants involving 10,000
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271 examples~\citep{Larochelle-jmlr-2009,VincentPLarochelleH2008-very-small}.
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272 The focus here is on much larger training sets, from 10 times to
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273 to 1000 times larger, and 62 classes.
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274
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275 The first step in constructing the larger datasets (called NISTP and P07) is to sample from
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276 a {\em data source}: {\bf NIST} (NIST database 19), {\bf Fonts}, {\bf Captchas},
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277 and {\bf OCR data} (scanned machine printed characters). See more in
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278 Section~\ref{sec:sources} below. Once a character
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279 is sampled from one of these sources (chosen randomly), the second step is to
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280 apply a pipeline of transformations and/or noise processes outlined in section \ref{s:perturbations}.
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281
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282 To provide a baseline of error rate comparison we also estimate human performance
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283 on both the 62-class task and the 10-class digits task.
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284 We compare the best Multi-Layer Perceptrons (MLP) against
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285 the best Stacked Denoising Auto-encoders (SDA), when
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286 both models' hyper-parameters are selected to minimize the validation set error.
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287 We also provide a comparison against a precise estimate
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288 of human performance obtained via Amazon's Mechanical Turk (AMT)
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289 service ({\tt http://mturk.com}).
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290 AMT users are paid small amounts
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291 of money to perform tasks for which human intelligence is required.
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292 Mechanical Turk has been used extensively in natural language processing and vision.
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293 %processing \citep{SnowEtAl2008} and vision
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294 %\citep{SorokinAndForsyth2008,whitehill09}.
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295 AMT users were presented
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296 with 10 character images (from a test set) on a screen
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297 and asked to label them.
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298 They were forced to choose a single character class (either among the
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299 62 or 10 character classes) for each image.
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300 80 subjects classified 2500 images per (dataset,task) pair.
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301 Different humans labelers sometimes provided a different label for the same
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302 example, and we were able to estimate the error variance due to this effect
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303 because each image was classified by 3 different persons.
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304 The average error of humans on the 62-class task NIST test set
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305 is 18.2\%, with a standard error of 0.1\%.
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306 We controlled noise in the labelling process by (1)
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307 requiring AMT workers with a higher than normal average of accepted
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308 responses ($>$95\%) on other tasks (2) discarding responses that were not
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309 complete (10 predictions) (3) discarding responses for which for which the
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310 time to predict was smaller than 3 seconds for NIST (the mean response time
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311 was 20 seconds) and 6 seconds seconds for NISTP (average response time of
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312 45 seconds) (4) discarding responses which were obviously wrong (10
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313 identical ones, or "12345..."). Overall, after such filtering, we kept
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314 approximately 95\% of the AMT workers' responses.
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315
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316 %\vspace*{-3mm}
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317 \subsection{Data Sources}
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318 \label{sec:sources}
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319 %\vspace*{-2mm}
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320
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321 %\begin{itemize}
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322 %\item
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323 {\bf NIST.}
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324 Our main source of characters is the NIST Special Database 19~\citep{Grother-1995},
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325 widely used for training and testing character
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326 recognition systems~\citep{Granger+al-2007,Cortes+al-2000,Oliveira+al-2002-short,Milgram+al-2005}.
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327 The dataset is composed of 814255 digits and characters (upper and lower cases), with hand checked classifications,
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328 extracted from handwritten sample forms of 3600 writers. The characters are labelled by one of the 62 classes
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329 corresponding to ``0''-``9'',``A''-``Z'' and ``a''-``z''. The dataset contains 8 parts (partitions) of varying complexity.
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330 The fourth partition (called $hsf_4$, 82,587 examples),
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331 experimentally recognized to be the most difficult one, is the one recommended
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332 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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333 for that purpose. We randomly split the remainder (731,668 examples) into a training set and a validation set for
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334 model selection.
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335 The performances reported by previous work on that dataset mostly use only the digits.
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336 Here we use all the classes both in the training and testing phase. This is especially
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337 useful to estimate the effect of a multi-task setting.
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338 The distribution of the classes in the NIST training and test sets differs
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339 substantially, with relatively many more digits in the test set, and a more uniform distribution
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340 of letters in the test set (whereas in the training set they are distributed
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341 more like in natural text).
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342 %\vspace*{-1mm}
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343
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344 %\item
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345 {\bf Fonts.}
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346 In order to have a good variety of sources we downloaded an important number of free fonts from:
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347 {\tt http://cg.scs.carleton.ca/\textasciitilde luc/freefonts.html}.
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348 % TODO: pointless to anonymize, it's not pointing to our work
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349 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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350 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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351 directly as input to our models.
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352 %\vspace*{-1mm}
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353
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354 %\item
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355 {\bf Captchas.}
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356 The Captcha data source is an adaptation of the \emph{pycaptcha} library (a Python-based captcha generator library) for
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357 generating characters of the same format as the NIST dataset. This software is based on
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358 a random character class generator and various kinds of transformations similar to those described in the previous sections.
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359 In order to increase the variability of the data generated, many different fonts are used for generating the characters.
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360 Transformations (slant, distortions, rotation, translation) are applied to each randomly generated character with a complexity
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361 depending on the value of the complexity parameter provided by the user of the data source.
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362 %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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363 %\vspace*{-1mm}
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364
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365 %\item
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366 {\bf OCR data.}
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367 A large set (2 million) of scanned, OCRed and manually verified machine-printed
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368 characters where included as an
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369 additional source. This set is part of a larger corpus being collected by the Image Understanding
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370 Pattern Recognition Research group led by Thomas Breuel at University of Kaiserslautern
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371 ({\tt http://www.iupr.com}), and which will be publicly released.
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372 %TODO: let's hope that Thomas is not a reviewer! :) Seriously though, maybe we should anonymize this
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373 %\end{itemize}
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374
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375 %\vspace*{-3mm}
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376 \subsection{Data Sets}
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377 %\vspace*{-2mm}
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378
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379 All data sets contain 32$\times$32 grey-level images (values in $[0,1]$) associated with a label
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380 from one of the 62 character classes.
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381 %\begin{itemize}
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382 %\vspace*{-1mm}
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383
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384 %\item
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385 {\bf NIST.} This is the raw NIST special database 19~\citep{Grother-1995}. It has
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386 \{651,668 / 80,000 / 82,587\} \{training / validation / test\} examples.
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387 %\vspace*{-1mm}
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388
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389 %\item
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390 {\bf P07.} This dataset is obtained by taking raw characters from all four of the above sources
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391 and sending them through the transformation pipeline described in section \ref{s:perturbations}.
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392 For each new example to generate, a data source is selected with probability $10\%$ from the fonts,
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393 $25\%$ from the captchas, $25\%$ from the OCR data and $40\%$ from NIST. We apply all the transformations in the
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394 order given above, and for each of them we sample uniformly a \emph{complexity} in the range $[0,0.7]$.
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395 It has \{81,920,000 / 80,000 / 20,000\} \{training / validation / test\} examples
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396 obtained from the corresponding NIST sets plus other sources.
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397 %\vspace*{-1mm}
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398
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399 %\item
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400 {\bf NISTP.} This one is equivalent to P07 (complexity parameter of $0.7$ with the same proportions of data sources)
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401 except that we only apply
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402 transformations from slant to pinch (see Fig.\ref{fig:transform}(b-f)).
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403 Therefore, the character is
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404 transformed but no additional noise is added to the image, giving images
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405 closer to the NIST dataset.
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406 It has \{81,920,000 / 80,000 / 20,000\} \{training / validation / test\} examples
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407 obtained from the corresponding NIST sets plus other sources.
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408 %\end{itemize}
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409
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410 \begin{figure*}[ht]
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411 %\vspace*{-2mm}
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412 \centerline{\resizebox{0.8\textwidth}{!}{\includegraphics{images/denoising_autoencoder_small.pdf}}}
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413 %\vspace*{-2mm}
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414 \caption{Illustration of the computations and training criterion for the denoising
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415 auto-encoder used to pre-train each layer of the deep architecture. Input $x$ of
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416 the layer (i.e. raw input or output of previous layer)
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417 s corrupted into $\tilde{x}$ and encoded into code $y$ by the encoder $f_\theta(\cdot)$.
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418 The decoder $g_{\theta'}(\cdot)$ maps $y$ to reconstruction $z$, which
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419 is compared to the uncorrupted input $x$ through the loss function
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420 $L_H(x,z)$, whose expected value is approximately minimized during training
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421 by tuning $\theta$ and $\theta'$.}
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422 \label{fig:da}
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423 %\vspace*{-2mm}
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424 \end{figure*}
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425
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426 %\vspace*{-3mm}
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427 \subsection{Models and their Hyper-parameters}
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428 %\vspace*{-2mm}
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429
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430 The experiments are performed using MLPs (with a single
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431 hidden layer) and deep SDAs.
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432 \emph{Hyper-parameters are selected based on the {\bf NISTP} validation set error.}
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433
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434 {\bf Multi-Layer Perceptrons (MLP).} The MLP output estimated with
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435 \[
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436 P({\rm class}|{\rm input}=x)={\rm softmax}(b_2+W_2\tanh(b_1+W_1 x)),
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437 \]
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438 i.e., two layers, where $p={\rm softmax}(a)$ means that
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439 $p_i(x)=\exp(a_i)/\sum_j \exp(a_j)$
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440 representing the probability
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441 for class $i$, $\tanh$ is the element-wise
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442 hyperbolic tangent, $b_i$ are parameter vectors, and $W_i$ are
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443 parameter matrices (one per layer). The
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444 number of rows of $W_1$ is called the number of hidden units (of the
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445 single hidden layer, here), and
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446 is one way to control capacity (the main other ways to control capacity are
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447 the number of training iterations and optionally a regularization penalty
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448 on the parameters, not used here because it did not help).
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449 Whereas previous work had compared
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450 deep architectures to both shallow MLPs and SVMs, we only compared to MLPs
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451 here because of the very large datasets used (making the use of SVMs
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452 computationally challenging because of their quadratic scaling
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453 behavior). Preliminary experiments on training SVMs (libSVM) with subsets
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454 of the training set allowing the program to fit in memory yielded
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455 substantially worse results than those obtained with MLPs\footnote{RBF SVMs
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456 trained with a subset of NISTP or NIST, 100k examples, to fit in memory,
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457 yielded 64\% test error or worse; online linear SVMs trained on the whole
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458 of NIST or 800k from NISTP yielded no better than 42\% error; slightly
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459 better results were obtained by sparsifying the pixel intensities and
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460 projecting to a second-order polynomial (a very sparse vector), still
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461 41\% error. We expect that better results could be obtained with a
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462 better implementation allowing for training with more examples and
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463 a higher-order non-linear projection.} For training on nearly a hundred million examples (with the
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464 perturbed data), the MLPs and SDA are much more convenient than classifiers
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465 based on kernel methods. The MLP has a single hidden layer with $\tanh$
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466 activation functions, and softmax (normalized exponentials) on the output
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467 layer for estimating $P({\rm class} | {\rm input})$. The number of hidden units is
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468 taken in $\{300,500,800,1000,1500\}$. Training examples are presented in
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469 minibatches of size 20, i.e., the parameters are iteratively updated in the direction
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470 of the mean gradient of the next 20 examples. A constant learning rate was chosen among $\{0.001,
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471 0.01, 0.025, 0.075, 0.1, 0.5\}$.
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472 %through preliminary experiments (measuring performance on a validation set),
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473 %and $0.1$ (which was found to work best) was then selected for optimizing on
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474 %the whole training sets.
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475 %\vspace*{-1mm}
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476
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477
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478 {\bf Stacked Denoising Auto-encoders (SDA).}
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479 Various auto-encoder variants and Restricted Boltzmann Machines (RBMs)
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480 can be used to initialize the weights of each layer of a deep MLP (with many hidden
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481 layers)~\citep{Hinton06,ranzato-07-small,Bengio-nips-2006},
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482 apparently setting parameters in the
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483 basin of attraction of supervised gradient descent yielding better
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484 generalization~\citep{Erhan+al-2010}. This initial {\em unsupervised
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485 pre-training phase} uses all of the training images but not the training labels.
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486 Each layer is trained in turn to produce a new representation of its input
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487 (starting from the raw pixels).
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488 It is hypothesized that the
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489 advantage brought by this procedure stems from a better prior,
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490 on the one hand taking advantage of the link between the input
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491 distribution $P(x)$ and the conditional distribution of interest
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492 $P(y|x)$ (like in semi-supervised learning), and on the other hand
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493 taking advantage of the expressive power and bias implicit in the
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494 deep architecture (whereby complex concepts are expressed as
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495 compositions of simpler ones through a deep hierarchy).
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496
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497 Here we chose to use the Denoising
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498 Auto-encoder~\citep{VincentPLarochelleH2008-very-small} as the building block for
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499 these deep hierarchies of features, as it is simple to train and
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500 explain (see Figure~\ref{fig:da}, as well as
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501 tutorial and code there: {\tt http://deeplearning.net/tutorial}),
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502 provides efficient inference, and yielded results
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503 comparable or better than RBMs in series of experiments
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504 \citep{VincentPLarochelleH2008-very-small}. It really corresponds to a Gaussian
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505 RBM trained by a Score Matching criterion~\cite{Vincent-SM-2010}.
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506 During its unsupervised training, a Denoising
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507 Auto-encoder is presented with a stochastically corrupted version $\tilde{x}$
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508 of the input $x$ and trained to reconstruct to produce a reconstruction $z$
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509 of the uncorrupted input $x$. Because the network has to denoise, it is
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510 forcing the hidden units $y$ to represent the leading regularities in
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511 the data. Following~\citep{VincentPLarochelleH2008-very-small}
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512 the hidden units output $y$ is obtained through the sigmoid-affine
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513 encoder
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514 \[
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515 y={\rm sigm}(c+V x)
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516 \]
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517 where ${\rm sigm}(a)=1/(1+\exp(-a))$
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518 and the reconstruction is obtained through the same transformation
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519 \[
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520 z={\rm sigm}(d+V' y)
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521 \]
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522 using the transpose of encoder weights.
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523 The training
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524 set average of the cross-entropy
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525 reconstruction loss
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diff changeset
526 \[
637
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527 L_H(x,z)=\sum_i z_i \log x_i + (1-z_i) \log(1-x_i)
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528 \]
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529 is minimized.
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diff changeset
530 Here we use the random binary masking corruption
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531 (which in $\tilde{x}$ sets to 0 a random subset of the elements of $x$, and
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diff changeset
532 copies the rest).
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parents: 630
diff changeset
533 Once the first denoising auto-encoder is trained, its parameters can be used
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534 to set the first layer of the deep MLP. The original data are then processed
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535 through that first layer, and the output of the hidden units form a new
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parents: 630
diff changeset
536 representation that can be used as input data for training a second denoising
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537 auto-encoder, still in a purely unsupervised way.
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diff changeset
538 This is repeated for the desired number of hidden layers.
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539 After this unsupervised pre-training stage, the parameters
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540 are used to initialize a deep MLP (similar to the above, but
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541 with more layers), which is fine-tuned by
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diff changeset
542 the same standard procedure (stochastic gradient descent)
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543 used to train MLPs in general (see above).
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544 The top layer parameters of the deep MLP (the one which outputs the
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545 class probabilities and takes the top hidden layer as input) can
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546 be initialized at 0.
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547 The SDA hyper-parameters are the same as for the MLP, with the addition of the
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548 amount of corruption noise (we used the masking noise process, whereby a
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549 fixed proportion of the input values, randomly selected, are zeroed), and a
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550 separate learning rate for the unsupervised pre-training stage (selected
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551 from the same above set). The fraction of inputs corrupted was selected
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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552 among $\{10\%, 20\%, 50\%\}$. Another hyper-parameter is the number
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diff changeset
553 of hidden layers but it was fixed to 3 for our experiments,
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554 based on previous work with
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555 SDAs on MNIST~\citep{VincentPLarochelleH2008-very-small}.
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diff changeset
556 We also compared against 1 and against 2 hidden layers,
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 636
diff changeset
557 to disantangle the effect of depth from that of unsupervised
627
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
558 pre-training.
637
fe98896745a5 fitting
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 636
diff changeset
559 The size of each hidden
fe98896745a5 fitting
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 636
diff changeset
560 layer was kept constant across hidden layers, and the best results
fe98896745a5 fitting
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 636
diff changeset
561 were obtained with the largest values that we tried
fe98896745a5 fitting
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 636
diff changeset
562 (1000 hidden units).
627
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
563
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
564 %\vspace*{-1mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
565
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
566 \begin{figure*}[ht]
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
567 %\vspace*{-2mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
568 \centerline{\resizebox{.99\textwidth}{!}{\includegraphics{images/error_rates_charts.pdf}}}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
569 %\vspace*{-3mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
570 \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
571 on NIST, 1 on NISTP, and 2 on P07. Left: overall results
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
572 of all models, on NIST and NISTP test sets.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
573 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
574 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
575 respectively based on ART, nearest neighbors, MLPs, and SVMs.}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
576 \label{fig:error-rates-charts}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
577 %\vspace*{-2mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
578 \end{figure*}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
579
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
580
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
581 \begin{figure*}[ht]
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
582 \vspace*{-3mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
583 \centerline{\resizebox{.99\textwidth}{!}{\includegraphics{images/improvements_charts.pdf}}}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
584 \vspace*{-3mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
585 \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
586 Left: Improvement (or loss, when negative)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
587 induced by out-of-distribution examples (perturbed data).
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
588 Right: Improvement (or loss, when negative) induced by multi-task
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
589 learning (training on all classes and testing only on either digits,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
590 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
591 out-of-distribution examples, compared to the shallow MLP.}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
592 \label{fig:improvements-charts}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
593 \vspace*{-2mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
594 \end{figure*}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
595
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
596 \vspace*{-2mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
597 \section{Experimental Results}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
598 \vspace*{-2mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
599
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
600 %%\vspace*{-1mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
601 %\subsection{SDA vs MLP vs Humans}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
602 %%\vspace*{-1mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
603 The models are either trained on NIST (MLP0 and SDA0),
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
604 NISTP (MLP1 and SDA1), or P07 (MLP2 and SDA2), and tested
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
605 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
606 either on the 62-class task
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
607 or on the 10-digits task. Training time (including about half
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
608 for unsupervised pre-training, for DAs) on the larger
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
609 datasets is around one day on a GPU (GTX 285).
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
610 Figure~\ref{fig:error-rates-charts} summarizes the results obtained,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
611 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
612 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
613 19 test set from the literature, respectively based on ARTMAP neural
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
614 networks ~\citep{Granger+al-2007}, fast nearest-neighbor search
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
615 ~\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
616 ~\citep{Milgram+al-2005}.% More detailed and complete numerical results
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
617 %(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
618 %found in Appendix.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
619 The deep learner not only outperformed the shallow ones and
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
620 previously published performance (in a statistically and qualitatively
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
621 significant way) but when trained with perturbed data
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
622 reaches human performance on both the 62-class task
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
623 and the 10-class (digits) task.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
624 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
625 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
626 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
627 ``c'' and a ``C'' are often indistinguishible).
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
628 Regarding shallower networks pre-trained with unsupervised denoising
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
629 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
630 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
631 with 3 hidden layers). Compare this with the 23\% error achieved
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
632 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
633 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
634 these results show that both depth and
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
635 unsupervised pre-training need to be combined in order to achieve
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
636 the best results.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
637
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
638
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
639 In addition, as shown in the left of
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
640 Figure~\ref{fig:improvements-charts}, the relative improvement in error
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
641 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
642 SDA, and these
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
643 differences with the shallow MLP are statistically and qualitatively
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
644 significant.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
645 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
646 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
647 (i.e. the perturbed examples examples from NISTP or P07),
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
648 over the models trained exclusively on NIST (respectively SDA0 and MLP0).
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
649 Relative percent change is measured by taking
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
650 $100 \% \times$ (original model's error / perturbed-data model's error - 1).
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
651 The right side of
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
652 Figure~\ref{fig:improvements-charts} shows the relative improvement
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
653 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
654 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
655 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
656 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
657 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
658 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
659 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
660 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
661 as $100\% \times$ (single-task
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
662 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
663 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
664 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
665 character classes as examples. Hence the hidden units are shared across
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
666 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
667 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
668 maximum conditional probability among only the digit classes outputs. The
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
669 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
670 and upper case characters). Note however that some types of perturbations
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
671 (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
672 %%\vspace*{-1mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
673 %\subsection{Perturbed Training Data More Helpful for SDA}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
674 %%\vspace*{-1mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
675
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
676 %%\vspace*{-1mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
677 %\subsection{Multi-Task Learning Effects}
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
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
680 \iffalse
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
681 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
682 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
683 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
684 recognizing upper case characters (knowing that the input is one), and
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
685 recognizing lower case characters (knowing that the input is one). We
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
686 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
687 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
688 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
689 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
690 (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
691 shallow learner.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
692
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
693 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
694 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
695 fine-tuned on NIST.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
696
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
697 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
698 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
699 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
700 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
701 error rate improvements of 27\%, 15\% and 13\% respectively for digits,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
702 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
703 \fi
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
704
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
705
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
706 \vspace*{-2mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
707 \section{Conclusions and Discussion}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
708 \vspace*{-2mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
709
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
710 We have found that out-of-distribution examples (multi-task learning
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
711 and perturbed examples) are more beneficial
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
712 to a deep learner than to a traditional shallow and purely
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
713 supervised learner. More precisely,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
714 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
715 %\begin{itemize}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
716
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
717 $\bullet$ %\item
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
718 {\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
719 MNIST digits generalize to a much larger and richer (but similar)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
720 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
721 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
722 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
723 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
724 and beating previously published results on the same data.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
725
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
726 $\bullet$ %\item
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
727 {\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
728 and do they help them more than shallow supervised ones}?
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
729 We found that distorted training examples not only made the resulting
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
730 classifier better on similarly perturbed images but also on
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
731 the {\em original clean examples}, and more importantly and more novel,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
732 that deep architectures benefit more from such {\em out-of-distribution}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
733 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
734 images (65\% relative improvement on NISTP)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
735 but only marginally helped (5\% relative improvement on all classes)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
736 or even hurt (10\% relative loss on digits)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
737 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
738 were significantly boosted by these out-of-distribution examples.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
739 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
740 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
741 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
742 which may be explained by the arguments below.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
743 Since out-of-distribution data
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
744 (perturbed or from other related classes) is very common, this conclusion
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
745 is of practical importance.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
746 %\end{itemize}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
747
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
748 In the original self-taught learning framework~\citep{RainaR2007}, the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
749 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
750 experiments showed its positive effects in a \emph{limited labeled data}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
751 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
752 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
753 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
754 We note instead that, for deep
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
755 architectures, our experiments show that such a positive effect is accomplished
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
756 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
757 i.e., here, the relative gain of self-taught learning and
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
758 out-of-distribution examples is probably preserved
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
759 in the asymptotic regime. However, note that in our perturbation experiments
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
760 (but not in our multi-task experiments),
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
761 even the out-of-distribution examples are labeled, unlike in the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
762 earlier self-taught learning experiments~\citep{RainaR2007}.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
763
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
764 {\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
765 framework and out-of-distribution examples}?
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
766 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
767 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
768 input distribution. A theoretical analysis of generalization improvements
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
769 due to sharing of intermediate features across tasks already points
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
770 towards that explanation~\cite{baxter95a}.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
771 Intermediate features that can be used in different
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
772 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
773 strength. Features extracted through many levels are more likely to
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
774 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
775 in the underlying distribution (as the experiments in~\citet{Goodfellow2009} suggest),
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
776 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
777 of tasks and input conditions.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
778 Therefore, we hypothesize that both depth and unsupervised
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
779 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
780 experiments could attempt at teasing apart these factors.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
781 And why would deep learners benefit from the self-taught learning
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
782 scenarios even when the number of labeled examples is very large?
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
783 We hypothesize that this is related to the hypotheses studied
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
784 in~\citet{Erhan+al-2010}. In~\citet{Erhan+al-2010}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
785 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
786 advantage of the deep learning bias vanish, and a similar phenomenon
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
787 may be happening here. We hypothesize that unsupervised pre-training
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
788 of a deep hierarchy with out-of-distribution examples initializes the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
789 model in the basin of attraction of supervised gradient descent
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
790 that corresponds to better generalization. Furthermore, such good
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
791 basins of attraction are not discovered by pure supervised learning
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
792 (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
793 does not allow the shallow or purely supervised models to discover
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
794 the kind of better basins associated
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
795 with deep learning and out-of-distribution examples.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
796
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
797 A Flash demo of the recognizer (where both the MLP and the SDA can be compared)
634
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 631
diff changeset
798 can be executed on-line at {\tt http://deep.host22.com}.
627
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
799
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
800 \iffalse
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
801 \section*{Appendix I: Detailed Numerical Results}
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 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
804 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
805
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
806 \begin{table}[ht]
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
807 \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
808 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
809 (SDA=Stacked Denoising Autoencoder) and ordinary shallow architecture
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
810 (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
811 and using a validation set to select hyper-parameters and other training choices.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
812 \{SDA,MLP\}0 are trained on NIST,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
813 \{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
814 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
815 recognized as letters. For comparison, the results found in the literature
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
816 on NIST digits classification using the same test set are included.}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
817 \label{tab:sda-vs-mlp-vs-humans}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
818 \begin{center}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
819 \begin{tabular}{|l|r|r|r|r|} \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
820 & NIST test & NISTP test & P07 test & NIST test digits \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
821 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
822 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
823 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
824 SDA2 & 18.7\% $\pm$.13\% & 33.6\%$\pm$.3\% & 39.9\%$\pm$.17\% & 1.7\% $\pm$.1\%\\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
825 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
826 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
827 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
828 \citep{Granger+al-2007} & & & & 4.95\% $\pm$.18\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
829 \citep{Cortes+al-2000} & & & & 3.71\% $\pm$.16\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
830 \citep{Oliveira+al-2002} & & & & 2.4\% $\pm$.13\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
831 \citep{Milgram+al-2005} & & & & 2.1\% $\pm$.12\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
832 \end{tabular}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
833 \end{center}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
834 \end{table}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
835
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
836 \begin{table}[ht]
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
837 \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
838 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
839 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
840 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
841 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
842 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
843 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
844 on the clean characters. }
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
845 \label{tab:perturbation-effect}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
846 \begin{center}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
847 \begin{tabular}{|l|r|r|r|r|} \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
848 & NIST test & NISTP test & P07 test & NIST test digits \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
849 SDA0/SDA1-1 & 38\% & 84\% & 228\% & 93\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
850 SDA0/SDA2-1 & 27\% & 94\% & 144\% & 59\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
851 MLP0/MLP1-1 & 5.2\% & 65\% & -13\% & -10\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
852 MLP0/MLP2-1 & -0.4\% & 49\% & 44\% & -29\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
853 \end{tabular}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
854 \end{center}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
855 \end{table}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
856
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
857 \begin{table}[ht]
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
858 \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
859 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
860 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
861 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
862 unperturbed NIST data, using validation error for model selection.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
863 Relative improvement is 1 - single-task error / multi-task error.}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
864 \label{tab:multi-task}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
865 \begin{center}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
866 \begin{tabular}{|l|r|r|r|} \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
867 & single-task & multi-task & relative \\
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
868 & setting & setting & improvement \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
869 MLP-digits & 3.77\% & 3.99\% & 5.6\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
870 MLP-lower & 17.4\% & 16.8\% & -4.1\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
871 MLP-upper & 7.84\% & 7.54\% & -3.6\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
872 SDA-digits & 2.6\% & 3.56\% & 27\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
873 SDA-lower & 12.3\% & 14.4\% & 15\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
874 SDA-upper & 5.93\% & 6.78\% & 13\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
875 \end{tabular}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
876 \end{center}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
877 \end{table}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
878
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
879 \fi
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
880
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
881 %\afterpage{\clearpage}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
882 %\clearpage
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
883 {
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
884 %\bibliographystyle{spbasic} % basic style, author-year citations
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
885 \bibliographystyle{plainnat}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
886 \bibliography{strings,strings-short,strings-shorter,ift6266_ml,specials,aigaion-shorter}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
887 %\bibliographystyle{unsrtnat}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
888 %\bibliographystyle{apalike}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
889 }
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
890
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
891
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
892 \end{document}