annotate writeup/aistats2011_cameraready.tex @ 628:ca20f94448dc

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author Yoshua Bengio <bengioy@iro.umontreal.ca>
date Thu, 17 Mar 2011 09:22:04 -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[numbers]{natbib}
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14
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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 Arnaud Bergeron \and
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31 Nicolas Boulanger-Lewandowski \and
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32 Thomas Breuel \and
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33 Youssouf Chherawala \and
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34 Moustapha Cisse \and
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35 Myriam Côté \and
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36 Dumitru Erhan \and
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37 Jeremy Eustache \and
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38 Xavier Glorot \and
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39 Xavier Muller \and
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40 Sylvain Pannetier Lebeuf \and
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41 Razvan Pascanu \and
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42 Salah Rifai \and
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43 Francois Savard \and
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44 Guillaume Sicard
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45 \vspace*{5mm}}]
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46 \aistatsaddress{Dept. IRO, U. Montreal, P.O. Box 6128, Centre-Ville branch, H3C 3J7, Montreal (Qc), Canada}
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47 %\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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48 %\jmlrheading{}{2010}{}{10/2010}{XX/2011}{Yoshua Bengio et al}
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49 %\editor{}
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50
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51 %\makeanontitle
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52 %\maketitle
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53
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54 %{\bf Running title: Deep Self-Taught Learning}
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55
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56 \vspace*{5mm}
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57 \begin{abstract}
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58 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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59 \end{abstract}
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60 %\vspace*{-3mm}
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61
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62 %\begin{keywords}
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63 %Deep learning, self-taught learning, out-of-distribution examples, handwritten character recognition, multi-task learning
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64 %\end{keywords}
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65 %\keywords{self-taught learning \and multi-task learning \and out-of-distribution examples \and deep learning \and handwriting recognition}
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66
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67
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68
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69 \section{Introduction}
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70 %\vspace*{-1mm}
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71
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72 {\bf Deep Learning} has emerged as a promising new area of research in
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73 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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74 Learning algorithms for deep architectures are centered on the learning
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75 of useful representations of data, which are better suited to the task at hand,
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76 and are organized in a hierarchy with multiple levels.
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77 This is in part inspired by observations of the mammalian visual cortex,
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78 which consists of a chain of processing elements, each of which is associated with a
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79 different representation of the raw visual input. In fact,
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80 it was found recently that the features learnt in deep architectures resemble
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81 those observed in the first two of these stages (in areas V1 and V2
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82 of visual cortex) \citep{HonglakL2008}, and that they become more and
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83 more invariant to factors of variation (such as camera movement) in
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84 higher layers~\citep{Goodfellow2009}.
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85 It has been hypothesized that learning a hierarchy of features increases the
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86 ease and practicality of developing representations that are at once
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87 tailored to specific tasks, yet are able to borrow statistical strength
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88 from other related tasks (e.g., modeling different kinds of objects). Finally, learning the
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89 feature representation can lead to higher-level (more abstract, more
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90 general) features that are more robust to unanticipated sources of
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91 variance extant in real data.
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92
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93 Whereas a deep architecture can in principle be more powerful than a
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94 shallow one in terms of representation, depth appears to render the
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95 training problem more difficult in terms of optimization and local minima.
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96 It is also only recently that successful algorithms were proposed to
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97 overcome some of these difficulties. All are based on unsupervised
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98 learning, often in an greedy layer-wise ``unsupervised pre-training''
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99 stage~\citep{Bengio-2009}.
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100 The principle is that each layer starting from
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101 the bottom is trained to represent its input (the output of the previous
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102 layer). After this
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103 unsupervised initialization, the stack of layers can be
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104 converted into a deep supervised feedforward neural network and fine-tuned by
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105 stochastic gradient descent.
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106 One of these layer initialization techniques,
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107 applied here, is the Denoising
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108 Auto-encoder~(DA)~\citep{VincentPLarochelleH2008-very-small} (see
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109 Figure~\ref{fig:da}), which performed similarly or
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110 better~\citep{VincentPLarochelleH2008-very-small} than previously
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111 proposed Restricted Boltzmann Machines (RBM)~\citep{Hinton06}
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112 in terms of unsupervised extraction
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113 of a hierarchy of features useful for classification. Each layer is trained
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114 to denoise its input, creating a layer of features that can be used as
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115 input for the next layer, forming a Stacked Denoising Auto-encoder (SDA).
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116 Note that training a Denoising Auto-encoder
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117 can actually been seen as training a particular RBM by an inductive
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118 principle different from maximum likelihood~\citep{Vincent-SM-2010},
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119 namely by Score Matching~\citep{Hyvarinen-2005,HyvarinenA2008}.
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120
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121 Previous comparative experimental results with stacking of RBMs and DAs
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122 to build deep supervised predictors had shown that they could outperform
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123 shallow architectures in a variety of settings, especially
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124 when the data involves complex interactions between many factors of
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125 variation~\citep{LarochelleH2007,Bengio-2009}. Other experiments have suggested
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126 that the unsupervised layer-wise pre-training acted as a useful
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127 prior~\citep{Erhan+al-2010} that allows one to initialize a deep
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128 neural network in a relatively much smaller region of parameter space,
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129 corresponding to better generalization.
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130
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131 To further the understanding of the reasons for the good performance
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132 observed with deep learners, we focus here on the following {\em hypothesis}:
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133 intermediate levels of representation, especially when there are
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134 more such levels, can be exploited to {\bf share
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135 statistical strength across different but related types of examples},
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136 such as examples coming from other tasks than the task of interest
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137 (the multi-task setting), or examples coming from an overlapping
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138 but different distribution (images with different kinds of perturbations
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139 and noises, here). This is consistent with the hypotheses discussed
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140 in~\citet{Bengio-2009} regarding the potential advantage
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141 of deep learning and the idea that more levels of representation can
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142 give rise to more abstract, more general features of the raw input.
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143
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144 This hypothesis is related to a learning setting called
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145 {\bf self-taught learning}~\citep{RainaR2007}, which combines principles
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146 of semi-supervised and multi-task learning: the learner can exploit examples
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147 that are unlabeled and possibly come from a distribution different from the target
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148 distribution, e.g., from other classes than those of interest.
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149 It has already been shown that deep learners can clearly take advantage of
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150 unsupervised learning and unlabeled examples~\citep{Bengio-2009,WestonJ2008-small},
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151 but more needed to be done to explore the impact
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152 of {\em out-of-distribution} examples and of the {\em multi-task} setting
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153 (one exception is~\citep{CollobertR2008}, which shares and uses unsupervised
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154 pre-training only with the first layer). In particular the {\em relative
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155 advantage of deep learning} for these settings has not been evaluated.
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156
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157
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158 %
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159 The {\bf main claim} of this paper is that deep learners (with several levels of representation) can
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160 {\bf benefit more from out-of-distribution examples than shallow learners} (with a single
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161 level), both in the context of the multi-task setting and from
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162 perturbed examples. Because we are able to improve on state-of-the-art
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163 performance and reach human-level performance
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164 on a large-scale task, we consider that this paper is also a contribution
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165 to advance the application of machine learning to handwritten character recognition.
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166 More precisely, we ask and answer the following questions:
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167
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168 %\begin{enumerate}
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169 $\bullet$ %\item
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170 Do the good results previously obtained with deep architectures on the
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171 MNIST digit images generalize to the setting of a similar but much larger and richer
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172 dataset, the NIST special database 19, with 62 classes and around 800k examples?
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173
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174 $\bullet$ %\item
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175 To what extent does the perturbation of input images (e.g. adding
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176 noise, affine transformations, background images) make the resulting
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177 classifiers better not only on similarly perturbed images but also on
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178 the {\em original clean examples}? We study this question in the
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179 context of the 62-class and 10-class tasks of the NIST special database 19.
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180
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181 $\bullet$ %\item
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182 Do deep architectures {\em benefit {\bf more} from such out-of-distribution}
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183 examples, in particular do they benefit more from
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184 examples that are perturbed versions of the examples from the task of interest?
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185
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186 $\bullet$ %\item
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187 Similarly, does the feature learning step in deep learning algorithms benefit {\bf more}
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188 from training with moderately {\em different classes} (i.e. a multi-task learning scenario) than
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189 a corresponding shallow and purely supervised architecture?
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190 We train on 62 classes and test on 10 (digits) or 26 (upper case or lower case)
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191 to answer this question.
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192 %\end{enumerate}
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193
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194 Our experimental results provide positive evidence towards all of these questions,
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195 as well as {\bf classifiers that reach human-level performance on 62-class isolated character
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196 recognition and beat previously published results on the NIST dataset (special database 19)}.
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197 To achieve these results, we introduce in the next section a sophisticated system
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198 for stochastically transforming character images and then explain the methodology,
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199 which is based on training with or without these transformed images and testing on
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200 clean ones.
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201 Code for generating these transformations as well as for the deep learning
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202 algorithms are made available at {\tt http://anonymous.url.net}.%{\tt http://hg.assembla.com/ift6266}.
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203
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204 %\vspace*{-3mm}
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205 %\newpage
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206 \section{Perturbed and Transformed Character Images}
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207 \label{s:perturbations}
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208 %\vspace*{-2mm}
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209
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210 Figure~\ref{fig:transform} shows the different transformations we used to stochastically
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211 transform $32 \times 32$ source images (such as the one in Fig.\ref{fig:torig})
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212 in order to obtain data from a larger distribution which
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213 covers a domain substantially larger than the clean characters distribution from
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214 which we start.
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215 Although character transformations have been used before to
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216 improve character recognizers, this effort is on a large scale both
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217 in number of classes and in the complexity of the transformations, hence
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218 in the complexity of the learning task.
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219 The code for these transformations (mostly Python) is available at
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220 {\tt http://anonymous.url.net}. All the modules in the pipeline (Figure~\ref{fig:transform}) share
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221 a global control parameter ($0 \le complexity \le 1$) that allows one to modulate the
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222 amount of deformation or noise introduced.
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223 There are two main parts in the pipeline. The first one,
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224 from thickness to pinch, performs transformations. The second
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225 part, from blur to contrast, adds different kinds of noise.
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226 More details can be found in~\citep{ift6266-tr-anonymous}.
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227
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228 \begin{figure*}[ht]
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229 \centering
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230 \subfigure[Original]{\includegraphics[scale=0.6]{images/Original.png}\label{fig:torig}}
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231 \subfigure[Thickness]{\includegraphics[scale=0.6]{images/Thick_only.png}}
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232 \subfigure[Slant]{\includegraphics[scale=0.6]{images/Slant_only.png}}
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233 \subfigure[Affine Transformation]{\includegraphics[scale=0.6]{images/Affine_only.png}}
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234 \subfigure[Local Elastic Deformation]{\includegraphics[scale=0.6]{images/Localelasticdistorsions_only.png}}
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235 \subfigure[Pinch]{\includegraphics[scale=0.6]{images/Pinch_only.png}}
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236 %Noise
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237 \subfigure[Motion Blur]{\includegraphics[scale=0.6]{images/Motionblur_only.png}}
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238 \subfigure[Occlusion]{\includegraphics[scale=0.6]{images/occlusion_only.png}}
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239 \subfigure[Gaussian Smoothing]{\includegraphics[scale=0.6]{images/Bruitgauss_only.png}}
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240 \subfigure[Pixels Permutation]{\includegraphics[scale=0.6]{images/Permutpixel_only.png}}
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241 \subfigure[Gaussian Noise]{\includegraphics[scale=0.6]{images/Distorsiongauss_only.png}}
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242 \subfigure[Background Image Addition]{\includegraphics[scale=0.6]{images/background_other_only.png}}
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243 \subfigure[Salt \& Pepper]{\includegraphics[scale=0.6]{images/Poivresel_only.png}}
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244 \subfigure[Scratches]{\includegraphics[scale=0.6]{images/Rature_only.png}}
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245 \subfigure[Grey Level \& Contrast]{\includegraphics[scale=0.6]{images/Contrast_only.png}}
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246 \caption{Top left (a): example original image. Others (b-o): examples of the effect
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247 of each transformation module taken separately. Actual perturbed examples are obtained by
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248 a pipeline of these, with random choices about which module to apply and how much perturbation
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249 to apply.}
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250 \label{fig:transform}
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251 %\vspace*{-2mm}
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252 \end{figure*}
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253
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254 %\vspace*{-3mm}
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255 \section{Experimental Setup}
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256 %\vspace*{-1mm}
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257
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258 Much previous work on deep learning had been performed on
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259 the MNIST digits task~\citep{Hinton06,ranzato-07-small,Bengio-nips-2006,Salakhutdinov+Hinton-2009},
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260 with 60,000 examples, and variants involving 10,000
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261 examples~\citep{Larochelle-jmlr-2009,VincentPLarochelleH2008-very-small}.
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262 The focus here is on much larger training sets, from 10 times to
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263 to 1000 times larger, and 62 classes.
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264
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265 The first step in constructing the larger datasets (called NISTP and P07) is to sample from
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266 a {\em data source}: {\bf NIST} (NIST database 19), {\bf Fonts}, {\bf Captchas},
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267 and {\bf OCR data} (scanned machine printed characters). See more in
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268 Section~\ref{sec:sources} below. Once a character
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269 is sampled from one of these sources (chosen randomly), the second step is to
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270 apply a pipeline of transformations and/or noise processes outlined in section \ref{s:perturbations}.
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271
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272 To provide a baseline of error rate comparison we also estimate human performance
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273 on both the 62-class task and the 10-class digits task.
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274 We compare the best Multi-Layer Perceptrons (MLP) against
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275 the best Stacked Denoising Auto-encoders (SDA), when
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276 both models' hyper-parameters are selected to minimize the validation set error.
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277 We also provide a comparison against a precise estimate
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278 of human performance obtained via Amazon's Mechanical Turk (AMT)
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279 service ({\tt http://mturk.com}).
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280 AMT users are paid small amounts
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281 of money to perform tasks for which human intelligence is required.
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282 Mechanical Turk has been used extensively in natural language processing and vision.
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283 %processing \citep{SnowEtAl2008} and vision
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284 %\citep{SorokinAndForsyth2008,whitehill09}.
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285 AMT users were presented
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286 with 10 character images (from a test set) on a screen
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287 and asked to label them.
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288 They were forced to choose a single character class (either among the
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289 62 or 10 character classes) for each image.
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290 80 subjects classified 2500 images per (dataset,task) pair.
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291 Different humans labelers sometimes provided a different label for the same
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292 example, and we were able to estimate the error variance due to this effect
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293 because each image was classified by 3 different persons.
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294 The average error of humans on the 62-class task NIST test set
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295 is 18.2\%, with a standard error of 0.1\%.
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296 We controlled noise in the labelling process by (1)
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297 requiring AMT workers with a higher than normal average of accepted
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298 responses ($>$95\%) on other tasks (2) discarding responses that were not
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299 complete (10 predictions) (3) discarding responses for which for which the
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300 time to predict was smaller than 3 seconds for NIST (the mean response time
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301 was 20 seconds) and 6 seconds seconds for NISTP (average response time of
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302 45 seconds) (4) discarding responses which were obviously wrong (10
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303 identical ones, or "12345..."). Overall, after such filtering, we kept
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304 approximately 95\% of the AMT workers' responses.
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305
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306 %\vspace*{-3mm}
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307 \subsection{Data Sources}
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308 \label{sec:sources}
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309 %\vspace*{-2mm}
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310
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311 %\begin{itemize}
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312 %\item
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313 {\bf NIST.}
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314 Our main source of characters is the NIST Special Database 19~\citep{Grother-1995},
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315 widely used for training and testing character
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316 recognition systems~\citep{Granger+al-2007,Cortes+al-2000,Oliveira+al-2002-short,Milgram+al-2005}.
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317 The dataset is composed of 814255 digits and characters (upper and lower cases), with hand checked classifications,
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318 extracted from handwritten sample forms of 3600 writers. The characters are labelled by one of the 62 classes
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319 corresponding to ``0''-``9'',``A''-``Z'' and ``a''-``z''. The dataset contains 8 parts (partitions) of varying complexity.
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320 The fourth partition (called $hsf_4$, 82,587 examples),
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321 experimentally recognized to be the most difficult one, is the one recommended
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322 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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323 for that purpose. We randomly split the remainder (731,668 examples) into a training set and a validation set for
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324 model selection.
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325 The performances reported by previous work on that dataset mostly use only the digits.
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326 Here we use all the classes both in the training and testing phase. This is especially
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327 useful to estimate the effect of a multi-task setting.
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328 The distribution of the classes in the NIST training and test sets differs
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329 substantially, with relatively many more digits in the test set, and a more uniform distribution
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330 of letters in the test set (whereas in the training set they are distributed
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331 more like in natural text).
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332 %\vspace*{-1mm}
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333
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334 %\item
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335 {\bf Fonts.}
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336 In order to have a good variety of sources we downloaded an important number of free fonts from:
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337 {\tt http://cg.scs.carleton.ca/\textasciitilde luc/freefonts.html}.
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338 % TODO: pointless to anonymize, it's not pointing to our work
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339 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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340 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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341 directly as input to our models.
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342 %\vspace*{-1mm}
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343
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344 %\item
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345 {\bf Captchas.}
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346 The Captcha data source is an adaptation of the \emph{pycaptcha} library (a Python-based captcha generator library) for
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347 generating characters of the same format as the NIST dataset. This software is based on
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348 a random character class generator and various kinds of transformations similar to those described in the previous sections.
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349 In order to increase the variability of the data generated, many different fonts are used for generating the characters.
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350 Transformations (slant, distortions, rotation, translation) are applied to each randomly generated character with a complexity
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351 depending on the value of the complexity parameter provided by the user of the data source.
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352 %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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353 %\vspace*{-1mm}
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354
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355 %\item
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356 {\bf OCR data.}
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357 A large set (2 million) of scanned, OCRed and manually verified machine-printed
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358 characters where included as an
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359 additional source. This set is part of a larger corpus being collected by the Image Understanding
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360 Pattern Recognition Research group led by Thomas Breuel at University of Kaiserslautern
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361 ({\tt http://www.iupr.com}), and which will be publicly released.
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362 %TODO: let's hope that Thomas is not a reviewer! :) Seriously though, maybe we should anonymize this
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363 %\end{itemize}
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364
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365 %\vspace*{-3mm}
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366 \subsection{Data Sets}
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367 %\vspace*{-2mm}
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368
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369 All data sets contain 32$\times$32 grey-level images (values in $[0,1]$) associated with a label
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370 from one of the 62 character classes.
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371 %\begin{itemize}
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372 %\vspace*{-1mm}
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373
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374 %\item
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375 {\bf NIST.} This is the raw NIST special database 19~\citep{Grother-1995}. It has
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376 \{651,668 / 80,000 / 82,587\} \{training / validation / test\} examples.
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377 %\vspace*{-1mm}
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378
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379 %\item
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380 {\bf P07.} This dataset is obtained by taking raw characters from all four of the above sources
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381 and sending them through the transformation pipeline described in section \ref{s:perturbations}.
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382 For each new example to generate, a data source is selected with probability $10\%$ from the fonts,
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383 $25\%$ from the captchas, $25\%$ from the OCR data and $40\%$ from NIST. We apply all the transformations in the
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384 order given above, and for each of them we sample uniformly a \emph{complexity} in the range $[0,0.7]$.
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385 It has \{81,920,000 / 80,000 / 20,000\} \{training / validation / test\} examples
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386 obtained from the corresponding NIST sets plus other sources.
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387 %\vspace*{-1mm}
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388
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389 %\item
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390 {\bf NISTP.} This one is equivalent to P07 (complexity parameter of $0.7$ with the same proportions of data sources)
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391 except that we only apply
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392 transformations from slant to pinch (see Fig.\ref{fig:transform}(b-f)).
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393 Therefore, the character is
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394 transformed but no additional noise is added to the image, giving images
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395 closer to the NIST dataset.
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396 It has \{81,920,000 / 80,000 / 20,000\} \{training / validation / test\} examples
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397 obtained from the corresponding NIST sets plus other sources.
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398 %\end{itemize}
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399
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400 \begin{figure*}[ht]
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401 %\vspace*{-2mm}
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402 \centerline{\resizebox{0.8\textwidth}{!}{\includegraphics{images/denoising_autoencoder_small.pdf}}}
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403 %\vspace*{-2mm}
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404 \caption{Illustration of the computations and training criterion for the denoising
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405 auto-encoder used to pre-train each layer of the deep architecture. Input $x$ of
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406 the layer (i.e. raw input or output of previous layer)
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407 s corrupted into $\tilde{x}$ and encoded into code $y$ by the encoder $f_\theta(\cdot)$.
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408 The decoder $g_{\theta'}(\cdot)$ maps $y$ to reconstruction $z$, which
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409 is compared to the uncorrupted input $x$ through the loss function
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410 $L_H(x,z)$, whose expected value is approximately minimized during training
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411 by tuning $\theta$ and $\theta'$.}
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412 \label{fig:da}
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413 %\vspace*{-2mm}
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414 \end{figure*}
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415
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416 %\vspace*{-3mm}
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417 \subsection{Models and their Hyper-parameters}
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418 %\vspace*{-2mm}
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419
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420 The experiments are performed using MLPs (with a single
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421 hidden layer) and deep SDAs.
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422 \emph{Hyper-parameters are selected based on the {\bf NISTP} validation set error.}
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423
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424 {\bf Multi-Layer Perceptrons (MLP).} Whereas previous work had compared
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425 deep architectures to both shallow MLPs and SVMs, we only compared to MLPs
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426 here because of the very large datasets used (making the use of SVMs
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427 computationally challenging because of their quadratic scaling
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428 behavior). Preliminary experiments on training SVMs (libSVM) with subsets
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429 of the training set allowing the program to fit in memory yielded
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430 substantially worse results than those obtained with MLPs\footnote{RBF SVMs
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431 trained with a subset of NISTP or NIST, 100k examples, to fit in memory,
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432 yielded 64\% test error or worse; online linear SVMs trained on the whole
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433 of NIST or 800k from NISTP yielded no better than 42\% error; slightly
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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434 better results were obtained by sparsifying the pixel intensities and
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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435 projecting to a second-order polynomial (a very sparse vector), still
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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436 41\% error. We expect that better results could be obtained with a
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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437 better implementation allowing for training with more examples and
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438 a higher-order non-linear projection.} For training on nearly a hundred million examples (with the
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439 perturbed data), the MLPs and SDA are much more convenient than classifiers
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440 based on kernel methods. The MLP has a single hidden layer with $\tanh$
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441 activation functions, and softmax (normalized exponentials) on the output
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442 layer for estimating $P(class | image)$. The number of hidden units is
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443 taken in $\{300,500,800,1000,1500\}$. Training examples are presented in
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444 minibatches of size 20. A constant learning rate was chosen among $\{0.001,
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445 0.01, 0.025, 0.075, 0.1, 0.5\}$.
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446 %through preliminary experiments (measuring performance on a validation set),
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447 %and $0.1$ (which was found to work best) was then selected for optimizing on
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448 %the whole training sets.
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449 %\vspace*{-1mm}
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450
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451
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452 {\bf Stacked Denoising Auto-encoders (SDA).}
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453 Various auto-encoder variants and Restricted Boltzmann Machines (RBMs)
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454 can be used to initialize the weights of each layer of a deep MLP (with many hidden
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455 layers)~\citep{Hinton06,ranzato-07-small,Bengio-nips-2006},
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456 apparently setting parameters in the
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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457 basin of attraction of supervised gradient descent yielding better
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458 generalization~\citep{Erhan+al-2010}. This initial {\em unsupervised
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459 pre-training phase} uses all of the training images but not the training labels.
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460 Each layer is trained in turn to produce a new representation of its input
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461 (starting from the raw pixels).
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462 It is hypothesized that the
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463 advantage brought by this procedure stems from a better prior,
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464 on the one hand taking advantage of the link between the input
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465 distribution $P(x)$ and the conditional distribution of interest
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466 $P(y|x)$ (like in semi-supervised learning), and on the other hand
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467 taking advantage of the expressive power and bias implicit in the
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468 deep architecture (whereby complex concepts are expressed as
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469 compositions of simpler ones through a deep hierarchy).
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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470
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471 Here we chose to use the Denoising
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472 Auto-encoder~\citep{VincentPLarochelleH2008-very-small} as the building block for
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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473 these deep hierarchies of features, as it is simple to train and
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474 explain (see Figure~\ref{fig:da}, as well as
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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475 tutorial and code there: {\tt http://deeplearning.net/tutorial}),
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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476 provides efficient inference, and yielded results
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477 comparable or better than RBMs in series of experiments
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478 \citep{VincentPLarochelleH2008-very-small}. It really corresponds to a Gaussian
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479 RBM trained by a Score Matching criterion~\cite{Vincent-SM-2010}.
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480 During training, a Denoising
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481 Auto-encoder is presented with a stochastically corrupted version
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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482 of the input and trained to reconstruct the uncorrupted input,
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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483 forcing the hidden units to represent the leading regularities in
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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484 the data. Here we use the random binary masking corruption
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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485 (which sets to 0 a random subset of the inputs).
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486 Once it is trained, in a purely unsupervised way,
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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487 its hidden units' activations can
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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488 be used as inputs for training a second one, etc.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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489 After this unsupervised pre-training stage, the parameters
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490 are used to initialize a deep MLP, which is fine-tuned by
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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491 the same standard procedure used to train them (see above).
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492 The SDA hyper-parameters are the same as for the MLP, with the addition of the
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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493 amount of corruption noise (we used the masking noise process, whereby a
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494 fixed proportion of the input values, randomly selected, are zeroed), and a
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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495 separate learning rate for the unsupervised pre-training stage (selected
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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496 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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497 among $\{10\%, 20\%, 50\%\}$. Another hyper-parameter is the number
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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498 of hidden layers but it was fixed to 3 for most experiments,
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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499 based on previous work with
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500 SDAs on MNIST~\citep{VincentPLarochelleH2008-very-small}.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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501 We also compared against 1 and against 2 hidden layers, in order
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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502 to disantangle the effect of depth from the effect of unsupervised
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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503 pre-training.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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504 The size of the hidden
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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505 layers was kept constant across hidden layers, and the best results
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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506 were obtained with the largest values that we could experiment
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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507 with given our patience, with 1000 hidden units.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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508
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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509 %\vspace*{-1mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
510
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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511 \begin{figure*}[ht]
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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512 %\vspace*{-2mm}
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513 \centerline{\resizebox{.99\textwidth}{!}{\includegraphics{images/error_rates_charts.pdf}}}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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514 %\vspace*{-3mm}
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515 \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>
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diff changeset
516 on NIST, 1 on NISTP, and 2 on P07. Left: overall results
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
517 of all models, on NIST and NISTP test sets.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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518 Right: error rates on NIST test digits only, along with the previous results from
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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519 literature~\citep{Granger+al-2007,Cortes+al-2000,Oliveira+al-2002-short,Milgram+al-2005}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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520 respectively based on ART, nearest neighbors, MLPs, and SVMs.}
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521 \label{fig:error-rates-charts}
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522 %\vspace*{-2mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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523 \end{figure*}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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524
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
525
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
526 \begin{figure*}[ht]
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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527 \vspace*{-3mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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528 \centerline{\resizebox{.99\textwidth}{!}{\includegraphics{images/improvements_charts.pdf}}}
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529 \vspace*{-3mm}
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parents:
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530 \caption{Relative improvement in error rate due to out-of-distribution examples.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
531 Left: Improvement (or loss, when negative)
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
532 induced by out-of-distribution examples (perturbed data).
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
533 Right: Improvement (or loss, when negative) induced by multi-task
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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534 learning (training on all classes and testing only on either digits,
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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535 upper case, or lower-case). The deep learner (SDA) benefits more from
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
536 out-of-distribution examples, compared to the shallow MLP.}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
537 \label{fig:improvements-charts}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
538 \vspace*{-2mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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539 \end{figure*}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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540
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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541 \vspace*{-2mm}
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542 \section{Experimental Results}
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543 \vspace*{-2mm}
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parents:
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544
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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545 %%\vspace*{-1mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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546 %\subsection{SDA vs MLP vs Humans}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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547 %%\vspace*{-1mm}
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548 The models are either trained on NIST (MLP0 and SDA0),
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diff changeset
549 NISTP (MLP1 and SDA1), or P07 (MLP2 and SDA2), and tested
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diff changeset
550 on either NIST, NISTP or P07 (regardless of the data set used for training),
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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diff changeset
551 either on the 62-class task
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parents:
diff changeset
552 or on the 10-digits task. Training time (including about half
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parents:
diff changeset
553 for unsupervised pre-training, for DAs) on the larger
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parents:
diff changeset
554 datasets is around one day on a GPU (GTX 285).
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
555 Figure~\ref{fig:error-rates-charts} summarizes the results obtained,
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parents:
diff changeset
556 comparing humans, the three MLPs (MLP0, MLP1, MLP2) and the three SDAs (SDA0, SDA1,
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diff changeset
557 SDA2), along with the previous results on the digits NIST special database
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
558 19 test set from the literature, respectively based on ARTMAP neural
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
559 networks ~\citep{Granger+al-2007}, fast nearest-neighbor search
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
560 ~\citep{Cortes+al-2000}, MLPs ~\citep{Oliveira+al-2002-short}, and SVMs
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
561 ~\citep{Milgram+al-2005}.% More detailed and complete numerical results
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
562 %(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
563 %found in Appendix.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
564 The deep learner not only outperformed the shallow ones and
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
565 previously published performance (in a statistically and qualitatively
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
566 significant way) but when trained with perturbed data
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
567 reaches human performance on both the 62-class task
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
568 and the 10-class (digits) task.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
569 17\% error (SDA1) or 18\% error (humans) may seem large but a large
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
570 majority of the errors from humans and from SDA1 are from out-of-context
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
571 confusions (e.g. a vertical bar can be a ``1'', an ``l'' or an ``L'', and a
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
572 ``c'' and a ``C'' are often indistinguishible).
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
573 Regarding shallower networks pre-trained with unsupervised denoising
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
574 auto-encders, we find that the NIST test error is 21\% with one hidden
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
575 layer and 20\% with two hidden layers (vs 17\% in the same conditions
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
576 with 3 hidden layers). Compare this with the 23\% error achieved
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
577 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
578 As found in previous work~\cite{Erhan+al-2010,Larochelle-jmlr-2009},
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
579 these results show that both depth and
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
580 unsupervised pre-training need to be combined in order to achieve
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
581 the best results.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
582
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
583
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
584 In addition, as shown in the left of
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
585 Figure~\ref{fig:improvements-charts}, the relative improvement in error
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
586 rate brought by out-of-distribution examples is greater for the deep
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
587 SDA, and these
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
588 differences with the shallow MLP are statistically and qualitatively
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
589 significant.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
590 The left side of the figure shows the improvement to the clean
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
591 NIST test set error brought by the use of out-of-distribution examples
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
592 (i.e. the perturbed examples examples from NISTP or P07),
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
593 over the models trained exclusively on NIST (respectively SDA0 and MLP0).
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
594 Relative percent change is measured by taking
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
595 $100 \% \times$ (original model's error / perturbed-data model's error - 1).
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
596 The right side of
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
597 Figure~\ref{fig:improvements-charts} shows the relative improvement
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
598 brought by the use of a multi-task setting, in which the same model is
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
599 trained for more classes than the target classes of interest (i.e. training
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
600 with all 62 classes when the target classes are respectively the digits,
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
601 lower-case, or upper-case characters). Again, whereas the gain from the
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
602 multi-task setting is marginal or negative for the MLP, it is substantial
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
603 for the SDA. Note that to simplify these multi-task experiments, only the original
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
604 NIST dataset is used. For example, the MLP-digits bar shows the relative
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
605 percent improvement in MLP error rate on the NIST digits test set
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
606 as $100\% \times$ (single-task
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
607 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
608 trained with only 10 outputs (one per digit), seeing only digit examples,
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
609 whereas the multi-task model is trained with 62 outputs, with all 62
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
610 character classes as examples. Hence the hidden units are shared across
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
611 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
612 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
613 maximum conditional probability among only the digit classes outputs. The
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
614 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
615 and upper case characters). Note however that some types of perturbations
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
616 (NISTP) help more than others (P07) when testing on the clean images.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
617 %%\vspace*{-1mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
618 %\subsection{Perturbed Training Data More Helpful for SDA}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
619 %%\vspace*{-1mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
620
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
621 %%\vspace*{-1mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
622 %\subsection{Multi-Task Learning Effects}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
623 %%\vspace*{-1mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
624
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
625 \iffalse
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
626 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
627 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
628 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
629 recognizing upper case characters (knowing that the input is one), and
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
630 recognizing lower case characters (knowing that the input is one). We
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
631 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
632 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
633 whether the effect is different for MLPs versus SDAs. The goal is to find
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
634 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
635 (i.e. the multi-task setting) compared to a corresponding purely supervised
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
636 shallow learner.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
637
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
638 We use a single hidden layer MLP with 1000 hidden units, and a SDA
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
639 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
640 fine-tuned on NIST.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
641
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
642 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
643 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
644 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
645 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
646 error rate improvements of 27\%, 15\% and 13\% respectively for digits,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
647 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
648 \fi
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
649
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
650
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
651 \vspace*{-2mm}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
652 \section{Conclusions and Discussion}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
653 \vspace*{-2mm}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
654
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
655 We have found that out-of-distribution examples (multi-task learning
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
656 and perturbed examples) are more beneficial
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
657 to a deep learner than to a traditional shallow and purely
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
658 supervised learner. More precisely,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
659 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
660 %\begin{itemize}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
661
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
662 $\bullet$ %\item
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
663 {\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
664 MNIST digits generalize to a much larger and richer (but similar)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
665 dataset, the NIST special database 19, with 62 classes and around 800k examples}?
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
666 Yes, the SDA {\em systematically outperformed the MLP and all the previously
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
667 published results on this dataset} (the ones that we are aware of), {\em in fact reaching human-level
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
668 performance} at around 17\% error on the 62-class task and 1.4\% on the digits,
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
669 and beating previously published results on the same data.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
670
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
671 $\bullet$ %\item
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
672 {\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
673 and do they help them more than shallow supervised ones}?
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
674 We found that distorted training examples not only made the resulting
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
675 classifier better on similarly perturbed images but also on
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
676 the {\em original clean examples}, and more importantly and more novel,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
677 that deep architectures benefit more from such {\em out-of-distribution}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
678 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
679 images (65\% relative improvement on NISTP)
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
680 but only marginally helped (5\% relative improvement on all classes)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
681 or even hurt (10\% relative loss on digits)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
682 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
683 were significantly boosted by these out-of-distribution examples.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
684 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
685 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
686 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
687 which may be explained by the arguments below.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
688 Since out-of-distribution data
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
689 (perturbed or from other related classes) is very common, this conclusion
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
690 is of practical importance.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
691 %\end{itemize}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
692
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
693 In the original self-taught learning framework~\citep{RainaR2007}, the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
694 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
695 experiments showed its positive effects in a \emph{limited labeled data}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
696 scenario. However, many of the results by \citet{RainaR2007} (who used a
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
697 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
698 learning vs ordinary supervised learning} diminishes as the number of labeled examples increases.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
699 We note instead that, for deep
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
700 architectures, our experiments show that such a positive effect is accomplished
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
701 even in a scenario with a \emph{large number of labeled examples},
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
702 i.e., here, the relative gain of self-taught learning and
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
703 out-of-distribution examples is probably preserved
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
704 in the asymptotic regime. However, note that in our perturbation experiments
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
705 (but not in our multi-task experiments),
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
706 even the out-of-distribution examples are labeled, unlike in the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
707 earlier self-taught learning experiments~\citep{RainaR2007}.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
708
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
709 {\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
710 framework and out-of-distribution examples}?
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
711 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
712 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
713 input distribution. A theoretical analysis of generalization improvements
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
714 due to sharing of intermediate features across tasks already points
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
715 towards that explanation~\cite{baxter95a}.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
716 Intermediate features that can be used in different
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
717 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
718 strength. Features extracted through many levels are more likely to
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
719 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
720 in the underlying distribution (as the experiments in~\citet{Goodfellow2009} suggest),
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
721 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
722 of tasks and input conditions.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
723 Therefore, we hypothesize that both depth and unsupervised
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
724 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
725 experiments could attempt at teasing apart these factors.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
726 And why would deep learners benefit from the self-taught learning
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
727 scenarios even when the number of labeled examples is very large?
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
728 We hypothesize that this is related to the hypotheses studied
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
729 in~\citet{Erhan+al-2010}. In~\citet{Erhan+al-2010}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
730 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
731 advantage of the deep learning bias vanish, and a similar phenomenon
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
732 may be happening here. We hypothesize that unsupervised pre-training
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
733 of a deep hierarchy with out-of-distribution examples initializes the
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
734 model in the basin of attraction of supervised gradient descent
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
735 that corresponds to better generalization. Furthermore, such good
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
736 basins of attraction are not discovered by pure supervised learning
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
737 (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
738 does not allow the shallow or purely supervised models to discover
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
739 the kind of better basins associated
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
740 with deep learning and out-of-distribution examples.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
741
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
742 A Flash demo of the recognizer (where both the MLP and the SDA can be compared)
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
743 can be executed on-line at the anonymous site {\tt http://deep.host22.com}.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
744
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
745 \iffalse
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
746 \section*{Appendix I: Detailed Numerical Results}
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 These tables correspond to Figures 2 and 3 and contain the raw error rates for each model and dataset considered.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
749 They also contain additional data such as test errors on P07 and standard errors.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
750
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
751 \begin{table}[ht]
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
752 \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
753 26 lower + 26 upper), except for last columns -- digits only, between deep architecture with pre-training
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
754 (SDA=Stacked Denoising Autoencoder) and ordinary shallow architecture
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
755 (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
756 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
757 \{SDA,MLP\}0 are trained on NIST,
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
758 \{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
759 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
760 recognized as letters. For comparison, the results found in the literature
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
761 on NIST digits classification using the same test set are included.}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
762 \label{tab:sda-vs-mlp-vs-humans}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
763 \begin{center}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
764 \begin{tabular}{|l|r|r|r|r|} \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
765 & NIST test & NISTP test & P07 test & NIST test digits \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
766 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
767 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
768 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
769 SDA2 & 18.7\% $\pm$.13\% & 33.6\%$\pm$.3\% & 39.9\%$\pm$.17\% & 1.7\% $\pm$.1\%\\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
770 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
771 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
772 MLP2 & 24.3\% $\pm$.15\% & 46.0\%$\pm$.35\% & 54.7\%$\pm$.17\% & 4.85\% $\pm$.18\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
773 \citep{Granger+al-2007} & & & & 4.95\% $\pm$.18\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
774 \citep{Cortes+al-2000} & & & & 3.71\% $\pm$.16\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
775 \citep{Oliveira+al-2002} & & & & 2.4\% $\pm$.13\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
776 \citep{Milgram+al-2005} & & & & 2.1\% $\pm$.12\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
777 \end{tabular}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
778 \end{center}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
779 \end{table}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
780
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
781 \begin{table}[ht]
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
782 \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
783 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
784 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
785 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
786 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
787 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
788 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
789 on the clean characters. }
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
790 \label{tab:perturbation-effect}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
791 \begin{center}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
792 \begin{tabular}{|l|r|r|r|r|} \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
793 & NIST test & NISTP test & P07 test & NIST test digits \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
794 SDA0/SDA1-1 & 38\% & 84\% & 228\% & 93\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
795 SDA0/SDA2-1 & 27\% & 94\% & 144\% & 59\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
796 MLP0/MLP1-1 & 5.2\% & 65\% & -13\% & -10\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
797 MLP0/MLP2-1 & -0.4\% & 49\% & 44\% & -29\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
798 \end{tabular}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
799 \end{center}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
800 \end{table}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
801
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
802 \begin{table}[ht]
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
803 \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
804 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
805 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
806 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
807 unperturbed NIST data, using validation error for model selection.
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
808 Relative improvement is 1 - single-task error / multi-task error.}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
809 \label{tab:multi-task}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
810 \begin{center}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
811 \begin{tabular}{|l|r|r|r|} \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
812 & single-task & multi-task & relative \\
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
813 & setting & setting & improvement \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
814 MLP-digits & 3.77\% & 3.99\% & 5.6\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
815 MLP-lower & 17.4\% & 16.8\% & -4.1\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
816 MLP-upper & 7.84\% & 7.54\% & -3.6\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
817 SDA-digits & 2.6\% & 3.56\% & 27\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
818 SDA-lower & 12.3\% & 14.4\% & 15\% \\ \hline
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
819 SDA-upper & 5.93\% & 6.78\% & 13\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
820 \end{tabular}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
821 \end{center}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
822 \end{table}
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
823
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
824 \fi
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
825
249a180795e3 camera ready version
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
826 %\afterpage{\clearpage}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
827 %\clearpage
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
828 {
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
829 %\bibliographystyle{spbasic} % basic style, author-year citations
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
830 \bibliographystyle{plainnat}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
831 \bibliography{strings,strings-short,strings-shorter,ift6266_ml,specials,aigaion-shorter}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
832 %\bibliographystyle{unsrtnat}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
833 %\bibliographystyle{apalike}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
834 }
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
835
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
836
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
837 \end{document}