Mercurial > ift6266
annotate writeup/nips2010_submission.tex @ 575:bff9ab360ef4
nips_rebuttal_clean
author | Yoshua Bengio <bengioy@iro.umontreal.ca> |
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date | Sat, 07 Aug 2010 22:46:12 -0400 |
parents | 9d01280ff1c1 |
children | df749e70f637 |
rev | line source |
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1 \documentclass{article} % For LaTeX2e |
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2 \usepackage{nips10submit_e,times} |
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3 \usepackage{wrapfig} |
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4 \usepackage{amsthm,amsmath,bbm} |
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5 \usepackage[psamsfonts]{amssymb} |
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6 \usepackage{algorithm,algorithmic} |
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7 \usepackage[utf8]{inputenc} |
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8 \usepackage{graphicx,subfigure} |
469 | 9 \usepackage[numbers]{natbib} |
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523 | 11 %\setlength\parindent{0mm} |
12 | |
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13 \title{Deep Self-Taught Learning for Handwritten Character Recognition} |
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14 \author{The IFT6266 Gang} |
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15 |
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16 \begin{document} |
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17 |
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18 %\makeanontitle |
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19 \maketitle |
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20 |
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21 \vspace*{-2mm} |
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22 \begin{abstract} |
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23 Recent theoretical and empirical work in statistical machine learning has |
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24 demonstrated the importance of learning algorithms for deep |
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25 architectures, i.e., function classes obtained by composing multiple |
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26 non-linear transformations. Self-taught learning (exploiting unlabeled |
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27 examples or examples from other distributions) has already been applied |
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28 to deep learners, but mostly to show the advantage of unlabeled |
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29 examples. Here we explore the advantage brought by {\em out-of-distribution examples}. |
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30 For this purpose we |
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31 developed a powerful generator of stochastic variations and noise |
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32 processes for character images, including not only affine transformations |
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33 but also slant, local elastic deformations, changes in thickness, |
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34 background images, grey level changes, contrast, occlusion, and various |
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35 types of noise. The out-of-distribution examples are obtained from these |
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36 highly distorted images or by including examples of object classes |
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37 different from those in the target test set. |
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38 We show that {\em deep learners benefit |
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39 more from them than a corresponding shallow learner}, at least in the area of |
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40 handwritten character recognition. In fact, we show that they reach |
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41 human-level performance on both handwritten digit classification and |
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42 62-class handwritten character recognition. |
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43 \end{abstract} |
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44 \vspace*{-3mm} |
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45 |
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46 \section{Introduction} |
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47 \vspace*{-1mm} |
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48 |
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49 {\bf Deep Learning} has emerged as a promising new area of research in |
469 | 50 statistical machine learning (see~\citet{Bengio-2009} for a review). |
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51 Learning algorithms for deep architectures are centered on the learning |
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52 of useful representations of data, which are better suited to the task at hand. |
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53 This is in part inspired by observations of the mammalian visual cortex, |
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54 which consists of a chain of processing elements, each of which is associated with a |
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55 different representation of the raw visual input. In fact, |
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56 it was found recently that the features learnt in deep architectures resemble |
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57 those observed in the first two of these stages (in areas V1 and V2 |
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58 of visual cortex)~\citep{HonglakL2008}, and that they become more and |
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59 more invariant to factors of variation (such as camera movement) in |
501 | 60 higher layers~\citep{Goodfellow2009}. |
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61 Learning a hierarchy of features increases the |
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62 ease and practicality of developing representations that are at once |
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63 tailored to specific tasks, yet are able to borrow statistical strength |
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64 from other related tasks (e.g., modeling different kinds of objects). Finally, learning the |
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65 feature representation can lead to higher-level (more abstract, more |
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66 general) features that are more robust to unanticipated sources of |
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67 variance extant in real data. |
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68 |
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69 {\bf Self-taught learning}~\citep{RainaR2007} is a paradigm that combines principles |
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70 of semi-supervised and multi-task learning: the learner can exploit examples |
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71 that are unlabeled and possibly come from a distribution different from the target |
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72 distribution, e.g., from other classes than those of interest. |
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73 It has already been shown that deep learners can clearly take advantage of |
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74 unsupervised learning and unlabeled examples~\citep{Bengio-2009,WestonJ2008-small}, |
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75 but more needs to be done to explore the impact |
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76 of {\em out-of-distribution} examples and of the multi-task setting |
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77 (one exception is~\citep{CollobertR2008}, which uses a different kind |
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78 of learning algorithm). In particular the {\em relative |
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79 advantage} of deep learning for these settings has not been evaluated. |
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80 The hypothesis discussed in the conclusion is that a deep hierarchy of features |
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81 may be better able to provide sharing of statistical strength |
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82 between different regions in input space or different tasks. |
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83 |
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84 \iffalse |
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85 Whereas a deep architecture can in principle be more powerful than a |
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86 shallow one in terms of representation, depth appears to render the |
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87 training problem more difficult in terms of optimization and local minima. |
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88 It is also only recently that successful algorithms were proposed to |
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89 overcome some of these difficulties. All are based on unsupervised |
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90 learning, often in an greedy layer-wise ``unsupervised pre-training'' |
469 | 91 stage~\citep{Bengio-2009}. One of these layer initialization techniques, |
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92 applied here, is the Denoising |
547 | 93 Auto-encoder~(DA)~\citep{VincentPLarochelleH2008-very-small} (see Figure~\ref{fig:da}), |
94 which | |
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95 performed similarly or better than previously proposed Restricted Boltzmann |
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96 Machines in terms of unsupervised extraction of a hierarchy of features |
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97 useful for classification. Each layer is trained to denoise its |
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98 input, creating a layer of features that can be used as input for the next layer. |
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99 \fi |
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100 %The principle is that each layer starting from |
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101 %the bottom is trained to encode its input (the output of the previous |
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102 %layer) and to reconstruct it from a corrupted version. After this |
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103 %unsupervised initialization, the stack of DAs 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 |
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107 % |
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108 In this paper we ask the following questions: |
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109 |
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110 %\begin{enumerate} |
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111 $\bullet$ %\item |
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112 Do the good results previously obtained with deep architectures on the |
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113 MNIST digit images generalize to the setting of a much larger and richer (but similar) |
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114 dataset, the NIST special database 19, with 62 classes and around 800k examples? |
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115 |
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116 $\bullet$ %\item |
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117 To what extent does the perturbation of input images (e.g. adding |
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118 noise, affine transformations, background images) make the resulting |
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119 classifiers better not only on similarly perturbed images but also on |
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120 the {\em original clean examples}? We study this question in the |
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121 context of the 62-class and 10-class tasks of the NIST special database 19. |
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122 |
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123 $\bullet$ %\item |
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124 Do deep architectures {\em benefit more from such out-of-distribution} |
469 | 125 examples, i.e. do they benefit more from the self-taught learning~\citep{RainaR2007} framework? |
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126 We use highly perturbed examples to generate out-of-distribution examples. |
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127 |
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128 $\bullet$ %\item |
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129 Similarly, does the feature learning step in deep learning algorithms benefit more |
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130 from training with moderately different classes (i.e. a multi-task learning scenario) than |
466
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131 a corresponding shallow and purely supervised architecture? |
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132 We train on 62 classes and test on 10 (digits) or 26 (upper case or lower case) |
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133 to answer this question. |
484
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134 %\end{enumerate} |
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135 |
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136 Our experimental results provide positive evidence towards all of these questions. |
547 | 137 To achieve these results, we introduce in the next section a sophisticated system |
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138 for stochastically transforming character images and then explain the methodology, |
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139 which is based on training with or without these transformed images and testing on |
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140 clean ones. We measure the relative advantage of out-of-distribution examples |
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141 for a deep learner vs a supervised shallow one. |
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142 Code for generating these transformations as well as for the deep learning |
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143 algorithms are made available. |
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144 We also estimate the relative advantage for deep learners of training with |
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145 other classes than those of interest, by comparing learners trained with |
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146 62 classes with learners trained with only a subset (on which they |
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147 are then tested). |
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148 The conclusion discusses |
547 | 149 the more general question of why deep learners may benefit so much from |
150 the self-taught learning framework. | |
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151 |
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152 \vspace*{-3mm} |
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153 \section{Perturbation and Transformation of Character Images} |
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154 \label{s:perturbations} |
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155 \vspace*{-2mm} |
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156 |
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157 \begin{wrapfigure}[8]{l}{0.15\textwidth} |
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158 %\begin{minipage}[b]{0.14\linewidth} |
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159 \vspace*{-5mm} |
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160 \begin{center} |
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161 \includegraphics[scale=.4]{images/Original.png}\\ |
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162 {\bf Original} |
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163 \end{center} |
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164 \end{wrapfigure} |
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165 %\vspace{0.7cm} |
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166 %\end{minipage}% |
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167 %\hspace{0.3cm}\begin{minipage}[b]{0.86\linewidth} |
467 | 168 This section describes the different transformations we used to stochastically |
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169 transform $32 \times 32$ source images (such as the one on the left) |
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170 in order to obtain data from a larger distribution which |
547 | 171 covers a domain substantially larger than the clean characters distribution from |
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172 which we start. |
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173 Although character transformations have been used before to |
547 | 174 improve character recognizers, this effort is on a large scale both |
175 in number of classes and in the complexity of the transformations, hence | |
176 in the complexity of the learning task. | |
177 More details can | |
469 | 178 be found in this technical report~\citep{ift6266-tr-anonymous}. |
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179 The code for these transformations (mostly python) is available at |
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180 {\tt http://anonymous.url.net}. All the modules in the pipeline share |
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181 a global control parameter ($0 \le complexity \le 1$) that allows one to modulate the |
467 | 182 amount of deformation or noise introduced. |
183 There are two main parts in the pipeline. The first one, | |
184 from slant to pinch below, performs transformations. The second | |
185 part, from blur to contrast, adds different kinds of noise. | |
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186 %\end{minipage} |
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187 |
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188 \vspace*{1mm} |
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189 %\subsection{Transformations} |
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190 {\large\bf 2.1 Transformations} |
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191 \vspace*{1mm} |
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192 |
501 | 193 |
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194 \begin{wrapfigure}[7]{l}{0.15\textwidth} |
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195 %\begin{minipage}[b]{0.14\linewidth} |
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196 %\centering |
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197 \begin{center} |
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198 \vspace*{-5mm} |
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199 \includegraphics[scale=.4]{images/Thick_only.png}\\ |
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200 {\bf Thickness} |
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201 \end{center} |
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202 %\vspace{.6cm} |
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203 %\end{minipage}% |
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204 %\hspace{0.3cm}\begin{minipage}[b]{0.86\linewidth} |
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205 \end{wrapfigure} |
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206 To change character {\bf thickness}, morphological operators of dilation and erosion~\citep{Haralick87,Serra82} |
467 | 207 are applied. The neighborhood of each pixel is multiplied |
208 element-wise with a {\em structuring element} matrix. | |
209 The pixel value is replaced by the maximum or the minimum of the resulting | |
210 matrix, respectively for dilation or erosion. Ten different structural elements with | |
211 increasing dimensions (largest is $5\times5$) were used. For each image, | |
212 randomly sample the operator type (dilation or erosion) with equal probability and one structural | |
541 | 213 element from a subset of the $n=round(m \times complexity)$ smallest structuring elements |
214 where $m=10$ for dilation and $m=6$ for erosion (to avoid completely erasing thin characters). | |
215 A neutral element (no transformation) | |
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216 is always present in the set. |
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217 %\vspace{.4cm} |
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218 %\end{minipage} |
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219 %\vspace{-.7cm} |
523 | 220 |
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221 \begin{minipage}[b]{0.14\linewidth} |
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222 \centering |
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223 \includegraphics[scale=.4]{images/Slant_only.png}\\ |
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224 {\bf Slant} |
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225 \end{minipage}% |
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226 \hspace{0.3cm} |
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227 \begin{minipage}[b]{0.83\linewidth} |
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228 %\centering |
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229 To produce {\bf slant}, each row of the image is shifted |
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230 proportionally to its height: $shift = round(slant \times height)$. |
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231 $slant \sim U[-complexity,complexity]$. |
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232 The shift is randomly chosen to be either to the left or to the right. |
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233 \vspace{1cm} |
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234 \end{minipage} |
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235 %\vspace*{-4mm} |
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236 |
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237 %\begin{minipage}[b]{0.14\linewidth} |
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238 %\centering |
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239 \begin{wrapfigure}[8]{l}{0.15\textwidth} |
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240 \vspace*{-6mm} |
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241 \begin{center} |
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242 \includegraphics[scale=.4]{images/Affine_only.png}\\ |
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243 {\small {\bf Affine \mbox{Transformation}}} |
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244 \end{center} |
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245 \end{wrapfigure} |
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246 %\end{minipage}% |
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247 %\hspace{0.3cm}\begin{minipage}[b]{0.86\linewidth} |
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248 A $2 \times 3$ {\bf affine transform} matrix (with |
555
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249 parameters $(a,b,c,d,e,f)$) is sampled according to the $complexity$. |
541 | 250 Output pixel $(x,y)$ takes the value of input pixel |
251 nearest to $(ax+by+c,dx+ey+f)$, | |
252 producing scaling, translation, rotation and shearing. | |
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253 Marginal distributions of $(a,b,c,d,e,f)$ have been tuned to |
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254 forbid large rotations (to avoid confusing classes) but to give good |
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255 variability of the transformation: $a$ and $d$ $\sim U[1-3 |
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256 complexity,1+3\,complexity]$, $b$ and $e$ $\sim U[-3 \,complexity,3\, |
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257 complexity]$, and $c$ and $f \sim U[-4 \,complexity, 4 \, |
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258 complexity]$.\\ |
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259 %\end{minipage} |
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260 |
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261 \vspace*{-4.5mm} |
523 | 262 |
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263 \begin{minipage}[t]{\linewidth} |
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264 \begin{wrapfigure}[7]{l}{0.15\textwidth} |
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265 %\hspace*{-8mm}\begin{minipage}[b]{0.25\linewidth} |
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266 %\centering |
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267 \begin{center} |
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268 \vspace*{-4mm} |
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269 \includegraphics[scale=.4]{images/Localelasticdistorsions_only.png}\\ |
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270 {\bf Local Elastic Deformation} |
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271 \end{center} |
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272 \end{wrapfigure} |
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273 %\end{minipage}% |
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274 %\hspace{-3mm}\begin{minipage}[b]{0.85\linewidth} |
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275 %\vspace*{-20mm} |
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276 The {\bf local elastic deformation} |
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277 module induces a ``wiggly'' effect in the image, following~\citet{SimardSP03-short}, |
467 | 278 which provides more details. |
541 | 279 The intensity of the displacement fields is given by |
280 $\alpha = \sqrt[3]{complexity} \times 10.0$, which are | |
281 convolved with a Gaussian 2D kernel (resulting in a blur) of | |
282 standard deviation $\sigma = 10 - 7 \times\sqrt[3]{complexity}$. | |
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283 %\vspace{.9cm} |
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284 \end{minipage} |
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285 |
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286 \vspace*{7mm} |
523 | 287 |
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288 %\begin{minipage}[b]{0.14\linewidth} |
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289 %\centering |
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290 \begin{wrapfigure}[7]{l}{0.15\textwidth} |
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291 \vspace*{-5mm} |
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292 \begin{center} |
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293 \includegraphics[scale=.4]{images/Pinch_only.png}\\ |
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294 {\bf Pinch} |
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295 \end{center} |
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296 \end{wrapfigure} |
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297 %\vspace{.6cm} |
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298 %\end{minipage}% |
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299 %\hspace{0.3cm}\begin{minipage}[b]{0.86\linewidth} |
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300 The {\bf pinch} module applies the ``Whirl and pinch'' GIMP filter with whirl set to 0. |
541 | 301 A pinch is ``similar to projecting the image onto an elastic |
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302 surface and pressing or pulling on the center of the surface'' (GIMP documentation manual). |
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303 For a square input image, draw a radius-$r$ disk |
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304 around its center $C$. Any pixel $P$ belonging to |
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305 that disk has its value replaced by |
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306 the value of a ``source'' pixel in the original image, |
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307 on the line that goes through $C$ and $P$, but |
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308 at some other distance $d_2$. Define $d_1=distance(P,C)$ |
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309 and $d_2 = sin(\frac{\pi{}d_1}{2r})^{-pinch} \times |
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310 d_1$, where $pinch$ is a parameter of the filter. |
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311 The actual value is given by bilinear interpolation considering the pixels |
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312 around the (non-integer) source position thus found. |
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313 Here $pinch \sim U[-complexity, 0.7 \times complexity]$. |
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314 %\vspace{1.5cm} |
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315 %\end{minipage} |
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316 |
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317 \vspace{1mm} |
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318 |
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319 {\large\bf 2.2 Injecting Noise} |
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320 %\subsection{Injecting Noise} |
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321 \vspace{2mm} |
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322 |
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323 %\vspace*{-.2cm} |
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324 \begin{minipage}[t]{0.14\linewidth} |
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325 \centering |
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326 \vspace*{-2mm} |
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327 \includegraphics[scale=.4]{images/Motionblur_only.png}\\ |
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328 {\bf Motion Blur} |
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329 \end{minipage}% |
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330 \hspace{0.3cm}\begin{minipage}[t]{0.83\linewidth} |
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331 %\vspace*{.5mm} |
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332 The {\bf motion blur} module is GIMP's ``linear motion blur'', which |
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333 has parameters $length$ and $angle$. The value of |
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334 a pixel in the final image is approximately the mean of the first $length$ pixels |
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335 found by moving in the $angle$ direction, |
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336 $angle \sim U[0,360]$ degrees, and $length \sim {\rm Normal}(0,(3 \times complexity)^2)$. |
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337 \vspace{5mm} |
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338 \end{minipage} |
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339 |
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340 \vspace*{1mm} |
523 | 341 |
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342 \begin{minipage}[t]{0.14\linewidth} |
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343 \centering |
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344 \includegraphics[scale=.4]{images/occlusion_only.png}\\ |
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345 {\bf Occlusion} |
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346 %\vspace{.5cm} |
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347 \end{minipage}% |
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348 \hspace{0.3cm}\begin{minipage}[t]{0.83\linewidth} |
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349 \vspace*{-18mm} |
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350 The {\bf occlusion} module selects a random rectangle from an {\em occluder} character |
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351 image and places it over the original {\em occluded} |
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352 image. Pixels are combined by taking the max(occluder, occluded), |
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353 i.e. keeping the lighter ones. |
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354 The rectangle corners |
467 | 355 are sampled so that larger complexity gives larger rectangles. |
356 The destination position in the occluded image are also sampled | |
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357 according to a normal distribution (more details in~\citet{ift6266-tr-anonymous}). |
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358 This module is skipped with probability 60\%. |
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359 %\vspace{7mm} |
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360 \end{minipage} |
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361 |
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362 \vspace*{1mm} |
523 | 363 |
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364 \begin{wrapfigure}[8]{l}{0.15\textwidth} |
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365 \vspace*{-6mm} |
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366 \begin{center} |
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367 %\begin{minipage}[t]{0.14\linewidth} |
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368 %\centering |
558
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369 \includegraphics[scale=.4]{images/Bruitgauss_only.png}\\ |
555
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370 {\bf Gaussian Smoothing} |
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371 \end{center} |
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372 \end{wrapfigure} |
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373 %\vspace{.5cm} |
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374 %\end{minipage}% |
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375 %\hspace{0.3cm}\begin{minipage}[t]{0.86\linewidth} |
557
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376 With the {\bf Gaussian smoothing} module, |
560
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377 different regions of the image are spatially smoothed. |
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378 This is achieved by first convolving |
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379 the image with an isotropic Gaussian kernel of |
495 | 380 size and variance chosen uniformly in the ranges $[12,12 + 20 \times |
560
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381 complexity]$ and $[2,2 + 6 \times complexity]$. This filtered image is normalized |
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382 between $0$ and $1$. We also create an isotropic weighted averaging window, of the |
464
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parents:
diff
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383 kernel size, with maximum value at the center. For each image we sample |
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nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
384 uniformly from $3$ to $3 + 10 \times complexity$ pixels that will be |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
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385 averaging centers between the original image and the filtered one. We |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
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386 initialize to zero a mask matrix of the image size. For each selected pixel |
560
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387 we add to the mask the averaging window centered on it. The final image is |
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388 computed from the following element-wise operation: $\frac{image + filtered\_image |
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389 \times mask}{mask+1}$. |
557
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390 This module is skipped with probability 75\%. |
555
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|
391 %\end{minipage} |
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392 |
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393 \newpage |
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394 |
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395 \vspace*{-9mm} |
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|
396 |
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397 %\hspace*{-3mm}\begin{minipage}[t]{0.18\linewidth} |
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398 %\centering |
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399 \begin{minipage}[t]{\linewidth} |
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400 \begin{wrapfigure}[7]{l}{0.15\textwidth} |
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401 \vspace*{-5mm} |
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402 \begin{center} |
558
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403 \includegraphics[scale=.4]{images/Permutpixel_only.png}\\ |
555
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parents:
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|
404 {\small\bf Permute Pixels} |
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405 \end{center} |
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parents:
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|
406 \end{wrapfigure} |
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parents:
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|
407 %\end{minipage}% |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
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|
408 %\hspace{-0cm}\begin{minipage}[t]{0.86\linewidth} |
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parents:
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changeset
|
409 %\vspace*{-20mm} |
560
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parents:
559
diff
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|
410 This module {\bf permutes neighbouring pixels}. It first selects a |
dc5c3f538a05
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Olivier Delalleau <delallea@iro>
parents:
559
diff
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|
411 fraction $\frac{complexity}{3}$ of pixels randomly in the image. Each |
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parents:
559
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changeset
|
412 of these pixels is then sequentially exchanged with a random pixel |
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Olivier Delalleau <delallea@iro>
parents:
559
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|
413 among its four nearest neighbors (on its left, right, top or bottom). |
557
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encore du visuel de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
diff
changeset
|
414 This module is skipped with probability 80\%.\\ |
555
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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|
415 \vspace*{1mm} |
551
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Frederic Bastien <nouiz@nouiz.org>
parents:
550
diff
changeset
|
416 \end{minipage} |
555
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parents:
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changeset
|
417 |
557
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
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|
418 \vspace{-3mm} |
523 | 419 |
555
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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diff
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|
420 \begin{minipage}[t]{\linewidth} |
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parents:
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|
421 \begin{wrapfigure}[7]{l}{0.15\textwidth} |
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
422 %\vspace*{-3mm} |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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diff
changeset
|
423 \begin{center} |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
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|
424 %\hspace*{-3mm}\begin{minipage}[t]{0.18\linewidth} |
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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diff
changeset
|
425 %\centering |
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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|
426 \vspace*{-5mm} |
558
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Olivier Delalleau <delallea@iro>
parents:
555
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changeset
|
427 \includegraphics[scale=.4]{images/Distorsiongauss_only.png}\\ |
555
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
428 {\small \bf Gauss. Noise} |
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parents:
554
diff
changeset
|
429 \end{center} |
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
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|
430 \end{wrapfigure} |
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parents:
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diff
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|
431 %\end{minipage}% |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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diff
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|
432 %\hspace{0.3cm}\begin{minipage}[t]{0.86\linewidth} |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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diff
changeset
|
433 \vspace*{12mm} |
557
17d16700e0c8
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
diff
changeset
|
434 The {\bf Gaussian noise} module simply adds, to each pixel of the image independently, a |
555
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
435 noise $\sim Normal(0,(\frac{complexity}{10})^2)$. |
557
17d16700e0c8
encore du visuel de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
diff
changeset
|
436 This module is skipped with probability 70\%. |
555
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
437 %\vspace{1.1cm} |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
438 \end{minipage} |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
439 |
557
17d16700e0c8
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
diff
changeset
|
440 \vspace*{1.2cm} |
555
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
441 |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
442 \begin{minipage}[t]{\linewidth} |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
443 \begin{minipage}[t]{0.14\linewidth} |
551
8f365abf171d
separete the transmo image
Frederic Bastien <nouiz@nouiz.org>
parents:
550
diff
changeset
|
444 \centering |
555
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
445 \includegraphics[scale=.4]{images/background_other_only.png}\\ |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
446 {\small \bf Bg Image} |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
447 \end{minipage}% |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
448 \hspace{0.3cm}\begin{minipage}[t]{0.83\linewidth} |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
449 \vspace*{-18mm} |
557
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
diff
changeset
|
450 Following~\citet{Larochelle-jmlr-2009}, the {\bf background image} module adds a random |
555
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
451 background image behind the letter, from a randomly chosen natural image, |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
452 with contrast adjustments depending on $complexity$, to preserve |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
453 more or less of the original character image. |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
454 %\vspace{.8cm} |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
455 \end{minipage} |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
456 \end{minipage} |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
457 %\vspace{-.7cm} |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
458 |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
459 \begin{minipage}[t]{0.14\linewidth} |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
460 \centering |
558
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Fixed compilation: .PNG -> .png
Olivier Delalleau <delallea@iro>
parents:
555
diff
changeset
|
461 \includegraphics[scale=.4]{images/Poivresel_only.png}\\ |
555
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
462 {\small \bf Salt \& Pepper} |
551
8f365abf171d
separete the transmo image
Frederic Bastien <nouiz@nouiz.org>
parents:
550
diff
changeset
|
463 \end{minipage}% |
555
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
464 \hspace{0.3cm}\begin{minipage}[t]{0.83\linewidth} |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
465 \vspace*{-18mm} |
557
17d16700e0c8
encore du visuel de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
diff
changeset
|
466 The {\bf salt and pepper noise} module adds noise $\sim U[0,1]$ to random subsets of pixels. |
555
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
467 The number of selected pixels is $0.2 \times complexity$. |
557
17d16700e0c8
encore du visuel de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
diff
changeset
|
468 This module is skipped with probability 75\%. |
555
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
469 %\vspace{.9cm} |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
470 \end{minipage} |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
471 %\vspace{-.7cm} |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
472 |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
473 \vspace{1mm} |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
474 |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
475 \begin{minipage}[t]{\linewidth} |
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
476 \begin{wrapfigure}[7]{l}{0.14\textwidth} |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
477 %\begin{minipage}[t]{0.14\linewidth} |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
478 %\centering |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
479 \begin{center} |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
480 \vspace*{-4mm} |
558
143a1467f157
Fixed compilation: .PNG -> .png
Olivier Delalleau <delallea@iro>
parents:
555
diff
changeset
|
481 \hspace*{-1mm}\includegraphics[scale=.4]{images/Rature_only.png}\\ |
555
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
482 {\bf Scratches} |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
483 %\end{minipage}% |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
484 \end{center} |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
485 \end{wrapfigure} |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
486 %\hspace{0.3cm}\begin{minipage}[t]{0.86\linewidth} |
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
487 %\vspace{.4cm} |
557
17d16700e0c8
encore du visuel de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
diff
changeset
|
488 The {\bf scratches} module places line-like white patches on the image. The |
517
0a5945249f2b
section 2, quick first pass
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
511
diff
changeset
|
489 lines are heavily transformed images of the digit ``1'' (one), chosen |
544
1cdfc17e890f
ca fitte maintenant
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
541
diff
changeset
|
490 at random among 500 such 1 images, |
467 | 491 randomly cropped and rotated by an angle $\sim Normal(0,(100 \times |
554 | 492 complexity)^2$ (in degrees), using bi-cubic interpolation. |
495 | 493 Two passes of a grey-scale morphological erosion filter |
467 | 494 are applied, reducing the width of the line |
495 by an amount controlled by $complexity$. | |
557
17d16700e0c8
encore du visuel de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
diff
changeset
|
496 This module is skipped with probability 85\%. The probabilities |
544
1cdfc17e890f
ca fitte maintenant
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
541
diff
changeset
|
497 of applying 1, 2, or 3 patches are (50\%,30\%,20\%). |
551
8f365abf171d
separete the transmo image
Frederic Bastien <nouiz@nouiz.org>
parents:
550
diff
changeset
|
498 \end{minipage} |
523 | 499 |
560
dc5c3f538a05
Small fixes (typos / precisions)
Olivier Delalleau <delallea@iro>
parents:
559
diff
changeset
|
500 \vspace*{1mm} |
555
b6dfba0a110c
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
501 |
557
17d16700e0c8
encore du visuel de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
diff
changeset
|
502 \begin{minipage}[t]{0.25\linewidth} |
551
8f365abf171d
separete the transmo image
Frederic Bastien <nouiz@nouiz.org>
parents:
550
diff
changeset
|
503 \centering |
559 | 504 \hspace*{-16mm}\includegraphics[scale=.4]{images/Contrast_only.png}\\ |
557
17d16700e0c8
encore du visuel de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
diff
changeset
|
505 {\bf Grey Level \& Contrast} |
551
8f365abf171d
separete the transmo image
Frederic Bastien <nouiz@nouiz.org>
parents:
550
diff
changeset
|
506 \end{minipage}% |
557
17d16700e0c8
encore du visuel de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
diff
changeset
|
507 \hspace{-12mm}\begin{minipage}[t]{0.82\linewidth} |
560
dc5c3f538a05
Small fixes (typos / precisions)
Olivier Delalleau <delallea@iro>
parents:
559
diff
changeset
|
508 \vspace*{-18mm} |
557
17d16700e0c8
encore du visuel de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
555
diff
changeset
|
509 The {\bf grey level and contrast} module changes the contrast by changing grey levels, and may invert the image polarity (white |
544
1cdfc17e890f
ca fitte maintenant
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
541
diff
changeset
|
510 to black and black to white). The contrast is $C \sim U[1-0.85 \times complexity,1]$ |
1cdfc17e890f
ca fitte maintenant
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
541
diff
changeset
|
511 so the image is normalized into $[\frac{1-C}{2},1-\frac{1-C}{2}]$. The |
1cdfc17e890f
ca fitte maintenant
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
541
diff
changeset
|
512 polarity is inverted with probability 50\%. |
555
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
513 %\vspace{.7cm} |
551
8f365abf171d
separete the transmo image
Frederic Bastien <nouiz@nouiz.org>
parents:
550
diff
changeset
|
514 \end{minipage} |
555
b6dfba0a110c
ameliorer l'aspect visuel, Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
554
diff
changeset
|
515 \vspace{2mm} |
551
8f365abf171d
separete the transmo image
Frederic Bastien <nouiz@nouiz.org>
parents:
550
diff
changeset
|
516 |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
517 |
499
2b58eda9fc08
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
495
diff
changeset
|
518 \iffalse |
523 | 519 \begin{figure}[ht] |
538 | 520 \centerline{\resizebox{.9\textwidth}{!}{\includegraphics{images/example_t.png}}}\\ |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
521 \caption{Illustration of the pipeline of stochastic |
519
eaa595ea2402
section 3 quickpass
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
518
diff
changeset
|
522 transformations applied to the image of a lower-case \emph{t} |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
523 (the upper left image). Each image in the pipeline (going from |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
524 left to right, first top line, then bottom line) shows the result |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
525 of applying one of the modules in the pipeline. The last image |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
526 (bottom right) is used as training example.} |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
527 \label{fig:pipeline} |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
528 \end{figure} |
499
2b58eda9fc08
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
495
diff
changeset
|
529 \fi |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
530 |
560
dc5c3f538a05
Small fixes (typos / precisions)
Olivier Delalleau <delallea@iro>
parents:
559
diff
changeset
|
531 \vspace*{-3mm} |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
532 \section{Experimental Setup} |
484
9a757d565e46
reduction de taille
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
483
diff
changeset
|
533 \vspace*{-1mm} |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
534 |
553
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
535 Much previous work on deep learning had been performed on |
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
536 the MNIST digits task~\citep{Hinton06,ranzato-07-small,Bengio-nips-2006,Salakhutdinov+Hinton-2009}, |
472 | 537 with 60~000 examples, and variants involving 10~000 |
553
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
538 examples~\citep{Larochelle-jmlr-toappear-2008,VincentPLarochelleH2008}. |
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
539 The focus here is on much larger training sets, from 10 times to |
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
540 to 1000 times larger, and 62 classes. |
530
8fe77eac344f
Clarifying the experimental setup, typos here and there
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
524
diff
changeset
|
541 |
535 | 542 The first step in constructing the larger datasets (called NISTP and P07) is to sample from |
499
2b58eda9fc08
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
495
diff
changeset
|
543 a {\em data source}: {\bf NIST} (NIST database 19), {\bf Fonts}, {\bf Captchas}, |
2b58eda9fc08
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
495
diff
changeset
|
544 and {\bf OCR data} (scanned machine printed characters). Once a character |
547 | 545 is sampled from one of these sources (chosen randomly), the second step is to |
546 apply a pipeline of transformations and/or noise processes described in section \ref{s:perturbations}. | |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
547 |
547 | 548 To provide a baseline of error rate comparison we also estimate human performance |
549 on both the 62-class task and the 10-class digits task. | |
566 | 550 We compare the best Multi-Layer Perceptrons (MLP) against |
551 the best Stacked Denoising Auto-encoders (SDA), when | |
552 both models' hyper-parameters are selected to minimize the validation set error. | |
553 We also provide a comparison against a precise estimate | |
502
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
554 of human performance obtained via Amazon's Mechanical Turk (AMT) |
530
8fe77eac344f
Clarifying the experimental setup, typos here and there
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
524
diff
changeset
|
555 service (http://mturk.com). |
502
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
556 AMT users are paid small amounts |
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
557 of money to perform tasks for which human intelligence is required. |
522
d41926a68993
remis les choses qui avaient disparu
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
521
diff
changeset
|
558 Mechanical Turk has been used extensively in natural language processing and vision. |
d41926a68993
remis les choses qui avaient disparu
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
521
diff
changeset
|
559 %processing \citep{SnowEtAl2008} and vision |
d41926a68993
remis les choses qui avaient disparu
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
521
diff
changeset
|
560 %\citep{SorokinAndForsyth2008,whitehill09}. |
530
8fe77eac344f
Clarifying the experimental setup, typos here and there
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
524
diff
changeset
|
561 AMT users were presented |
553
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
562 with 10 character images (from a test set) and asked to choose 10 corresponding ASCII |
569
9d01280ff1c1
commentaires de Joseph Turian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
568
diff
changeset
|
563 characters. They were forced to choose a single character class (either among the |
9d01280ff1c1
commentaires de Joseph Turian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
568
diff
changeset
|
564 62 or 10 character classes) for each image. |
553
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
565 80 subjects classified 2500 images per (dataset,task) pair, |
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
566 with the guarantee that 3 different subjects classified each image, allowing |
550
662299f265ab
suggestions from Ian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
549
diff
changeset
|
567 us to estimate inter-human variability (e.g a standard error of 0.1\% |
553
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
568 on the average 18.2\% error done by humans on the 62-class task NIST test set). |
502
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
569 |
553
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
570 \vspace*{-3mm} |
472 | 571 \subsection{Data Sources} |
553
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
572 \vspace*{-2mm} |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
573 |
484
9a757d565e46
reduction de taille
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
483
diff
changeset
|
574 %\begin{itemize} |
9a757d565e46
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
483
diff
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|
575 %\item |
9a757d565e46
reduction de taille
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
483
diff
changeset
|
576 {\bf NIST.} |
501 | 577 Our main source of characters is the NIST Special Database 19~\citep{Grother-1995}, |
472 | 578 widely used for training and testing character |
516
092dae9a5040
make the reference more compact.
Frederic Bastien <nouiz@nouiz.org>
parents:
514
diff
changeset
|
579 recognition systems~\citep{Granger+al-2007,Cortes+al-2000,Oliveira+al-2002-short,Milgram+al-2005}. |
519
eaa595ea2402
section 3 quickpass
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
518
diff
changeset
|
580 The dataset is composed of 814255 digits and characters (upper and lower cases), with hand checked classifications, |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
581 extracted from handwritten sample forms of 3600 writers. The characters are labelled by one of the 62 classes |
519
eaa595ea2402
section 3 quickpass
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
518
diff
changeset
|
582 corresponding to ``0''-``9'',``A''-``Z'' and ``a''-``z''. The dataset contains 8 parts (partitions) of varying complexity. |
534 | 583 The fourth partition (called $hsf_4$, 82587 examples), |
584 experimentally recognized to be the most difficult one, is the one recommended | |
519
eaa595ea2402
section 3 quickpass
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
518
diff
changeset
|
585 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} |
534 | 586 for that purpose. We randomly split the remainder (731668 examples) into a training set and a validation set for |
587 model selection. | |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
588 The performances reported by previous work on that dataset mostly use only the digits. |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
589 Here we use all the classes both in the training and testing phase. This is especially |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
590 useful to estimate the effect of a multi-task setting. |
553
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
591 The distribution of the classes in the NIST training and test sets differs |
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
592 substantially, with relatively many more digits in the test set, and a more uniform distribution |
566 | 593 of letters in the test set (whereas in the training set they are distributed |
553
8f6c09d1140f
ca fitte de nouveau
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
552
diff
changeset
|
594 more like in natural text). |
549 | 595 \vspace*{-1mm} |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
596 |
484
9a757d565e46
reduction de taille
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
483
diff
changeset
|
597 %\item |
9a757d565e46
reduction de taille
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
483
diff
changeset
|
598 {\bf Fonts.} |
519
eaa595ea2402
section 3 quickpass
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
518
diff
changeset
|
599 In order to have a good variety of sources we downloaded an important number of free fonts from: |
530
8fe77eac344f
Clarifying the experimental setup, typos here and there
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
524
diff
changeset
|
600 {\tt http://cg.scs.carleton.ca/\textasciitilde luc/freefonts.html}. |
519
eaa595ea2402
section 3 quickpass
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
518
diff
changeset
|
601 % TODO: pointless to anonymize, it's not pointing to our work |
530
8fe77eac344f
Clarifying the experimental setup, typos here and there
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
524
diff
changeset
|
602 Including the operating system's (Windows 7) fonts, there is a total of $9817$ different fonts that we can choose uniformly from. |
8fe77eac344f
Clarifying the experimental setup, typos here and there
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
524
diff
changeset
|
603 The chosen {\tt ttf} file is either used as input of the Captcha generator (see next item) or, by producing a corresponding image, |
479
6593e67381a3
Added transformation figure
Xavier Glorot <glorotxa@iro.umontreal.ca>
parents:
476
diff
changeset
|
604 directly as input to our models. |
549 | 605 \vspace*{-1mm} |
479
6593e67381a3
Added transformation figure
Xavier Glorot <glorotxa@iro.umontreal.ca>
parents:
476
diff
changeset
|
606 |
484
9a757d565e46
reduction de taille
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
483
diff
changeset
|
607 %\item |
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608 {\bf Captchas.} |
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609 The Captcha data source is an adaptation of the \emph{pycaptcha} library (a python based captcha generator library) for |
472 | 610 generating characters of the same format as the NIST dataset. This software is based on |
495 | 611 a random character class generator and various kinds of transformations similar to those described in the previous sections. |
472 | 612 In order to increase the variability of the data generated, many different fonts are used for generating the characters. |
495 | 613 Transformations (slant, distortions, rotation, translation) are applied to each randomly generated character with a complexity |
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614 depending on the value of the complexity parameter provided by the user of the data source. |
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615 %Two levels of complexity are allowed and can be controlled via an easy to use facade class. %TODO: what's a facade class? |
549 | 616 \vspace*{-1mm} |
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617 |
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618 %\item |
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619 {\bf OCR data.} |
472 | 620 A large set (2 million) of scanned, OCRed and manually verified machine-printed |
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621 characters where included as an |
472 | 622 additional source. This set is part of a larger corpus being collected by the Image Understanding |
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623 Pattern Recognition Research group led by Thomas Breuel at University of Kaiserslautern |
495 | 624 ({\tt http://www.iupr.com}), and which will be publicly released. |
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625 %TODO: let's hope that Thomas is not a reviewer! :) Seriously though, maybe we should anonymize this |
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626 %\end{itemize} |
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627 |
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628 \vspace*{-3mm} |
472 | 629 \subsection{Data Sets} |
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630 \vspace*{-2mm} |
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631 |
472 | 632 All data sets contain 32$\times$32 grey-level images (values in $[0,1]$) associated with a label |
633 from one of the 62 character classes. | |
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634 %\begin{itemize} |
549 | 635 \vspace*{-1mm} |
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636 |
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637 %\item |
534 | 638 {\bf NIST.} This is the raw NIST special database 19~\citep{Grother-1995}. It has |
535 | 639 \{651668 / 80000 / 82587\} \{training / validation / test\} examples. |
549 | 640 \vspace*{-1mm} |
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641 |
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642 %\item |
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643 {\bf P07.} This dataset is obtained by taking raw characters from all four of the above sources |
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644 and sending them through the transformation pipeline described in section \ref{s:perturbations}. |
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645 For each new example to generate, a data source is selected with probability $10\%$ from the fonts, |
472 | 646 $25\%$ from the captchas, $25\%$ from the OCR data and $40\%$ from NIST. We apply all the transformations in the |
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647 order given above, and for each of them we sample uniformly a \emph{complexity} in the range $[0,0.7]$. |
535 | 648 It has \{81920000 / 80000 / 20000\} \{training / validation / test\} examples. |
549 | 649 \vspace*{-1mm} |
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650 |
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651 %\item |
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652 {\bf NISTP.} This one is equivalent to P07 (complexity parameter of $0.7$ with the same proportions of data sources) |
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653 except that we only apply |
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654 transformations from slant to pinch. Therefore, the character is |
495 | 655 transformed but no additional noise is added to the image, giving images |
534 | 656 closer to the NIST dataset. |
535 | 657 It has \{81920000 / 80000 / 20000\} \{training / validation / test\} examples. |
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658 %\end{itemize} |
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659 |
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660 \vspace*{-3mm} |
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661 \subsection{Models and their Hyperparameters} |
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662 \vspace*{-2mm} |
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663 |
566 | 664 The experiments are performed using MLPs (with a single |
665 hidden layer) and SDAs. | |
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666 \emph{Hyper-parameters are selected based on the {\bf NISTP} validation set error.} |
472 | 667 |
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668 {\bf Multi-Layer Perceptrons (MLP).} |
472 | 669 Whereas previous work had compared deep architectures to both shallow MLPs and |
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670 SVMs, we only compared to MLPs here because of the very large datasets used |
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671 (making the use of SVMs computationally challenging because of their quadratic |
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672 scaling behavior). |
472 | 673 The MLP has a single hidden layer with $\tanh$ activation functions, and softmax (normalized |
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674 exponentials) on the output layer for estimating $P(class | image)$. |
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675 The number of hidden units is taken in $\{300,500,800,1000,1500\}$. |
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676 Training examples are presented in minibatches of size 20. A constant learning |
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677 rate was chosen among $\{0.001, 0.01, 0.025, 0.075, 0.1, 0.5\}$. |
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678 %through preliminary experiments (measuring performance on a validation set), |
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679 %and $0.1$ (which was found to work best) was then selected for optimizing on |
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680 %the whole training sets. |
549 | 681 \vspace*{-1mm} |
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682 |
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683 |
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684 {\bf Stacked Denoising Auto-Encoders (SDA).} |
472 | 685 Various auto-encoder variants and Restricted Boltzmann Machines (RBMs) |
686 can be used to initialize the weights of each layer of a deep MLP (with many hidden | |
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687 layers)~\citep{Hinton06,ranzato-07-small,Bengio-nips-2006}, |
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688 apparently setting parameters in the |
472 | 689 basin of attraction of supervised gradient descent yielding better |
690 generalization~\citep{Erhan+al-2010}. It is hypothesized that the | |
691 advantage brought by this procedure stems from a better prior, | |
692 on the one hand taking advantage of the link between the input | |
693 distribution $P(x)$ and the conditional distribution of interest | |
694 $P(y|x)$ (like in semi-supervised learning), and on the other hand | |
695 taking advantage of the expressive power and bias implicit in the | |
696 deep architecture (whereby complex concepts are expressed as | |
697 compositions of simpler ones through a deep hierarchy). | |
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698 |
547 | 699 \begin{figure}[ht] |
700 \vspace*{-2mm} | |
701 \centerline{\resizebox{0.8\textwidth}{!}{\includegraphics{images/denoising_autoencoder_small.pdf}}} | |
549 | 702 \vspace*{-2mm} |
547 | 703 \caption{Illustration of the computations and training criterion for the denoising |
704 auto-encoder used to pre-train each layer of the deep architecture. Input $x$ of | |
705 the layer (i.e. raw input or output of previous layer) | |
569
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706 s corrupted into $\tilde{x}$ and encoded into code $y$ by the encoder $f_\theta(\cdot)$. |
547 | 707 The decoder $g_{\theta'}(\cdot)$ maps $y$ to reconstruction $z$, which |
708 is compared to the uncorrupted input $x$ through the loss function | |
709 $L_H(x,z)$, whose expected value is approximately minimized during training | |
710 by tuning $\theta$ and $\theta'$.} | |
711 \label{fig:da} | |
712 \vspace*{-2mm} | |
713 \end{figure} | |
714 | |
472 | 715 Here we chose to use the Denoising |
566 | 716 Auto-encoder~\citep{VincentPLarochelleH2008} as the building block for |
569
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717 these deep hierarchies of features, as it is simple to train and |
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718 explain (see Figure~\ref{fig:da}, as well as |
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719 tutorial and code there: {\tt http://deeplearning.net/tutorial}), |
566 | 720 provides efficient inference, and yielded results |
472 | 721 comparable or better than RBMs in series of experiments |
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722 \citep{VincentPLarochelleH2008}. During training, a Denoising |
566 | 723 Auto-encoder is presented with a stochastically corrupted version |
472 | 724 of the input and trained to reconstruct the uncorrupted input, |
725 forcing the hidden units to represent the leading regularities in | |
569
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726 the data. Here we use the random binary masking corruption |
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727 (which sets to 0 a random subset of the inputs). |
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728 Once it is trained, in a purely unsupervised way, |
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729 its hidden units' activations can |
472 | 730 be used as inputs for training a second one, etc. |
731 After this unsupervised pre-training stage, the parameters | |
732 are used to initialize a deep MLP, which is fine-tuned by | |
733 the same standard procedure used to train them (see previous section). | |
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734 The SDA hyper-parameters are the same as for the MLP, with the addition of the |
472 | 735 amount of corruption noise (we used the masking noise process, whereby a |
736 fixed proportion of the input values, randomly selected, are zeroed), and a | |
737 separate learning rate for the unsupervised pre-training stage (selected | |
738 from the same above set). The fraction of inputs corrupted was selected | |
739 among $\{10\%, 20\%, 50\%\}$. Another hyper-parameter is the number | |
740 of hidden layers but it was fixed to 3 based on previous work with | |
547 | 741 SDAs on MNIST~\citep{VincentPLarochelleH2008}. |
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742 |
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743 \vspace*{-1mm} |
523 | 744 |
745 \begin{figure}[ht] | |
541 | 746 \vspace*{-2mm} |
523 | 747 \centerline{\resizebox{.99\textwidth}{!}{\includegraphics{images/error_rates_charts.pdf}}} |
549 | 748 \vspace*{-3mm} |
547 | 749 \caption{SDAx are the {\bf deep} models. Error bars indicate a 95\% confidence interval. 0 indicates that the model was trained |
523 | 750 on NIST, 1 on NISTP, and 2 on P07. Left: overall results |
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751 of all models, on NIST and NISTP test sets. |
523 | 752 Right: error rates on NIST test digits only, along with the previous results from |
753 literature~\citep{Granger+al-2007,Cortes+al-2000,Oliveira+al-2002-short,Milgram+al-2005} | |
754 respectively based on ART, nearest neighbors, MLPs, and SVMs.} | |
755 \label{fig:error-rates-charts} | |
541 | 756 \vspace*{-2mm} |
523 | 757 \end{figure} |
758 | |
759 | |
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760 \begin{figure}[ht] |
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761 \vspace*{-3mm} |
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762 \centerline{\resizebox{.99\textwidth}{!}{\includegraphics{images/improvements_charts.pdf}}} |
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763 \vspace*{-3mm} |
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764 \caption{Relative improvement in error rate due to self-taught learning. |
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765 Left: Improvement (or loss, when negative) |
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766 induced by out-of-distribution examples (perturbed data). |
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767 Right: Improvement (or loss, when negative) induced by multi-task |
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768 learning (training on all classes and testing only on either digits, |
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769 upper case, or lower-case). The deep learner (SDA) benefits more from |
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770 both self-taught learning scenarios, compared to the shallow MLP.} |
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771 \label{fig:improvements-charts} |
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772 \vspace*{-2mm} |
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773 \end{figure} |
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774 |
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775 \section{Experimental Results} |
549 | 776 \vspace*{-2mm} |
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777 |
485
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778 %\vspace*{-1mm} |
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779 %\subsection{SDA vs MLP vs Humans} |
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780 %\vspace*{-1mm} |
535 | 781 The models are either trained on NIST (MLP0 and SDA0), |
782 NISTP (MLP1 and SDA1), or P07 (MLP2 and SDA2), and tested | |
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783 on either NIST, NISTP or P07, either on the 62-class task |
568 | 784 or on the 10-digits task. Training (including about half |
785 for unsupervised pre-training, for DAs) on the larger | |
786 datasets takes around one day on a GPU-285. | |
485
6beaf3328521
les tables enlevées
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
484
diff
changeset
|
787 Figure~\ref{fig:error-rates-charts} summarizes the results obtained, |
550
662299f265ab
suggestions from Ian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
549
diff
changeset
|
788 comparing humans, the three MLPs (MLP0, MLP1, MLP2) and the three SDAs (SDA0, SDA1, |
486
877af97ee193
section resultats et appendice
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
485
diff
changeset
|
789 SDA2), along with the previous results on the digits NIST special database |
566 | 790 19 test set from the literature, respectively based on ARTMAP neural |
486
877af97ee193
section resultats et appendice
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
485
diff
changeset
|
791 networks ~\citep{Granger+al-2007}, fast nearest-neighbor search |
516
092dae9a5040
make the reference more compact.
Frederic Bastien <nouiz@nouiz.org>
parents:
514
diff
changeset
|
792 ~\citep{Cortes+al-2000}, MLPs ~\citep{Oliveira+al-2002-short}, and SVMs |
486
877af97ee193
section resultats et appendice
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
485
diff
changeset
|
793 ~\citep{Milgram+al-2005}. More detailed and complete numerical results |
493
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
794 (figures and tables, including standard errors on the error rates) can be |
535 | 795 found in Appendix I of the supplementary material. |
796 The deep learner not only outperformed the shallow ones and | |
493
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
797 previously published performance (in a statistically and qualitatively |
535 | 798 significant way) but when trained with perturbed data |
799 reaches human performance on both the 62-class task | |
523 | 800 and the 10-class (digits) task. |
550
662299f265ab
suggestions from Ian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
549
diff
changeset
|
801 17\% error (SDA1) or 18\% error (humans) may seem large but a large |
662299f265ab
suggestions from Ian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
549
diff
changeset
|
802 majority of the errors from humans and from SDA1 are from out-of-context |
662299f265ab
suggestions from Ian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
549
diff
changeset
|
803 confusions (e.g. a vertical bar can be a ``1'', an ``l'' or an ``L'', and a |
662299f265ab
suggestions from Ian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
549
diff
changeset
|
804 ``c'' and a ``C'' are often indistinguishible). |
523 | 805 |
806 In addition, as shown in the left of | |
807 Figure~\ref{fig:improvements-charts}, the relative improvement in error | |
493
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
808 rate brought by self-taught learning is greater for the SDA, and these |
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
809 differences with the MLP are statistically and qualitatively |
502
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
810 significant. |
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
811 The left side of the figure shows the improvement to the clean |
493
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
812 NIST test set error brought by the use of out-of-distribution examples |
502
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
813 (i.e. the perturbed examples examples from NISTP or P07). |
547 | 814 Relative percent change is measured by taking |
548
34cb28249de0
suggestions de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
547
diff
changeset
|
815 $100 \% \times$ (original model's error / perturbed-data model's error - 1). |
502
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
816 The right side of |
523 | 817 Figure~\ref{fig:improvements-charts} shows the relative improvement |
486
877af97ee193
section resultats et appendice
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
485
diff
changeset
|
818 brought by the use of a multi-task setting, in which the same model is |
877af97ee193
section resultats et appendice
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
485
diff
changeset
|
819 trained for more classes than the target classes of interest (i.e. training |
877af97ee193
section resultats et appendice
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
485
diff
changeset
|
820 with all 62 classes when the target classes are respectively the digits, |
493
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
821 lower-case, or upper-case characters). Again, whereas the gain from the |
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
822 multi-task setting is marginal or negative for the MLP, it is substantial |
547 | 823 for the SDA. Note that to simplify these multi-task experiments, only the original |
493
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
824 NIST dataset is used. For example, the MLP-digits bar shows the relative |
547 | 825 percent improvement in MLP error rate on the NIST digits test set |
566 | 826 is $100\% \times$ (single-task |
827 model's error / multi-task model's error - 1). The single-task model is | |
493
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
828 trained with only 10 outputs (one per digit), seeing only digit examples, |
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
829 whereas the multi-task model is trained with 62 outputs, with all 62 |
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
830 character classes as examples. Hence the hidden units are shared across |
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
831 all tasks. For the multi-task model, the digit error rate is measured by |
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
832 comparing the correct digit class with the output class associated with the |
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
833 maximum conditional probability among only the digit classes outputs. The |
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
834 setting is similar for the other two target classes (lower case characters |
a194ce5a4249
difference stat. sign.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
491
diff
changeset
|
835 and upper case characters). |
485
6beaf3328521
les tables enlevées
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
484
diff
changeset
|
836 %\vspace*{-1mm} |
502
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
837 %\subsection{Perturbed Training Data More Helpful for SDA} |
485
6beaf3328521
les tables enlevées
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
484
diff
changeset
|
838 %\vspace*{-1mm} |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
839 |
485
6beaf3328521
les tables enlevées
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
484
diff
changeset
|
840 %\vspace*{-1mm} |
6beaf3328521
les tables enlevées
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
484
diff
changeset
|
841 %\subsection{Multi-Task Learning Effects} |
6beaf3328521
les tables enlevées
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
484
diff
changeset
|
842 %\vspace*{-1mm} |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
843 |
485
6beaf3328521
les tables enlevées
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
484
diff
changeset
|
844 \iffalse |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
845 As previously seen, the SDA is better able to benefit from the |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
846 transformations applied to the data than the MLP. In this experiment we |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
847 define three tasks: recognizing digits (knowing that the input is a digit), |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
848 recognizing upper case characters (knowing that the input is one), and |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
849 recognizing lower case characters (knowing that the input is one). We |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
850 consider the digit classification task as the target task and we want to |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
851 evaluate whether training with the other tasks can help or hurt, and |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
852 whether the effect is different for MLPs versus SDAs. The goal is to find |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
853 out if deep learning can benefit more (or less) from multiple related tasks |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
854 (i.e. the multi-task setting) compared to a corresponding purely supervised |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
855 shallow learner. |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
856 |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
857 We use a single hidden layer MLP with 1000 hidden units, and a SDA |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
858 with 3 hidden layers (1000 hidden units per layer), pre-trained and |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
859 fine-tuned on NIST. |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
860 |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
861 Our results show that the MLP benefits marginally from the multi-task setting |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
862 in the case of digits (5\% relative improvement) but is actually hurt in the case |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
863 of characters (respectively 3\% and 4\% worse for lower and upper class characters). |
495 | 864 On the other hand the SDA benefited from the multi-task setting, with relative |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
865 error rate improvements of 27\%, 15\% and 13\% respectively for digits, |
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
866 lower and upper case characters, as shown in Table~\ref{tab:multi-task}. |
485
6beaf3328521
les tables enlevées
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
484
diff
changeset
|
867 \fi |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
changeset
|
868 |
475 | 869 |
549 | 870 \vspace*{-2mm} |
529 | 871 \section{Conclusions and Discussion} |
549 | 872 \vspace*{-2mm} |
464
24f4a8b53fcc
nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff
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|
873 |
502
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changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
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|
874 We have found that the self-taught learning framework is more beneficial |
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
875 to a deep learner than to a traditional shallow and purely |
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
876 supervised learner. More precisely, |
520
18a6379999fd
more after lunch :)
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
519
diff
changeset
|
877 the answers are positive for all the questions asked in the introduction. |
484
9a757d565e46
reduction de taille
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
483
diff
changeset
|
878 %\begin{itemize} |
487 | 879 |
484
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reduction de taille
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
483
diff
changeset
|
880 $\bullet$ %\item |
547 | 881 {\bf Do the good results previously obtained with deep architectures on the |
549 | 882 MNIST digits generalize to a much larger and richer (but similar) |
547 | 883 dataset, the NIST special database 19, with 62 classes and around 800k examples}? |
569
9d01280ff1c1
commentaires de Joseph Turian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
568
diff
changeset
|
884 Yes, the SDA {\em systematically outperformed the MLP and all the previously |
9d01280ff1c1
commentaires de Joseph Turian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
568
diff
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|
885 published results on this dataset} (the ones that we are aware of), {\em in fact reaching human-level |
529 | 886 performance} at around 17\% error on the 62-class task and 1.4\% on the digits. |
484
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parents:
483
diff
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|
887 |
9a757d565e46
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parents:
483
diff
changeset
|
888 $\bullet$ %\item |
547 | 889 {\bf To what extent do self-taught learning scenarios help deep learners, |
890 and do they help them more than shallow supervised ones}? | |
529 | 891 We found that distorted training examples not only made the resulting |
892 classifier better on similarly perturbed images but also on | |
893 the {\em original clean examples}, and more importantly and more novel, | |
894 that deep architectures benefit more from such {\em out-of-distribution} | |
895 examples. MLPs were helped by perturbed training examples when tested on perturbed input | |
502
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changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
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|
896 images (65\% relative improvement on NISTP) |
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
897 but only marginally helped (5\% relative improvement on all classes) |
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
898 or even hurt (10\% relative loss on digits) |
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
899 with respect to clean examples . On the other hand, the deep SDAs |
569
9d01280ff1c1
commentaires de Joseph Turian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
568
diff
changeset
|
900 were significantly boosted by these out-of-distribution examples. |
529 | 901 Similarly, whereas the improvement due to the multi-task setting was marginal or |
502
2b35a6e5ece4
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
902 negative for the MLP (from +5.6\% to -3.6\% relative change), |
569
9d01280ff1c1
commentaires de Joseph Turian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
568
diff
changeset
|
903 it was quite significant for the SDA (from +13\% to +27\% relative change), |
547 | 904 which may be explained by the arguments below. |
484
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
483
diff
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|
905 %\end{itemize} |
472 | 906 |
524
07bc0ca8d246
added paragraph comparing "our" self-taught learning with "theirs"
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
523
diff
changeset
|
907 In the original self-taught learning framework~\citep{RainaR2007}, the |
07bc0ca8d246
added paragraph comparing "our" self-taught learning with "theirs"
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
523
diff
changeset
|
908 out-of-sample examples were used as a source of unsupervised data, and |
07bc0ca8d246
added paragraph comparing "our" self-taught learning with "theirs"
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
523
diff
changeset
|
909 experiments showed its positive effects in a \emph{limited labeled data} |
07bc0ca8d246
added paragraph comparing "our" self-taught learning with "theirs"
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
523
diff
changeset
|
910 scenario. However, many of the results by \citet{RainaR2007} (who used a |
550
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
549
diff
changeset
|
911 shallow, sparse coding approach) suggest that the {\em relative gain of self-taught |
662299f265ab
suggestions from Ian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
549
diff
changeset
|
912 learning vs ordinary supervised learning} diminishes as the number of labeled examples increases. |
662299f265ab
suggestions from Ian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
549
diff
changeset
|
913 We note instead that, for deep |
524
07bc0ca8d246
added paragraph comparing "our" self-taught learning with "theirs"
Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
523
diff
changeset
|
914 architectures, our experiments show that such a positive effect is accomplished |
569
9d01280ff1c1
commentaires de Joseph Turian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
568
diff
changeset
|
915 even in a scenario with a \emph{large number of labeled examples}, |
550
662299f265ab
suggestions from Ian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
549
diff
changeset
|
916 i.e., here, the relative gain of self-taught learning is probably preserved |
662299f265ab
suggestions from Ian
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
549
diff
changeset
|
917 in the asymptotic regime. |
524
07bc0ca8d246
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Dumitru Erhan <dumitru.erhan@gmail.com>
parents:
523
diff
changeset
|
918 |
547 | 919 {\bf Why would deep learners benefit more from the self-taught learning framework}? |
502
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
920 The key idea is that the lower layers of the predictor compute a hierarchy |
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
921 of features that can be shared across tasks or across variants of the |
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
501
diff
changeset
|
922 input distribution. Intermediate features that can be used in different |
2b35a6e5ece4
changements de Myriam
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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923 contexts can be estimated in a way that allows to share statistical |
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924 strength. Features extracted through many levels are more likely to |
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925 be more abstract (as the experiments in~\citet{Goodfellow2009} suggest), |
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926 increasing the likelihood that they would be useful for a larger array |
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927 of tasks and input conditions. |
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928 Therefore, we hypothesize that both depth and unsupervised |
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929 pre-training play a part in explaining the advantages observed here, and future |
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930 experiments could attempt at teasing apart these factors. |
529 | 931 And why would deep learners benefit from the self-taught learning |
932 scenarios even when the number of labeled examples is very large? | |
933 We hypothesize that this is related to the hypotheses studied | |
934 in~\citet{Erhan+al-2010}. Whereas in~\citet{Erhan+al-2010} | |
935 it was found that online learning on a huge dataset did not make the | |
936 advantage of the deep learning bias vanish, a similar phenomenon | |
937 may be happening here. We hypothesize that unsupervised pre-training | |
938 of a deep hierarchy with self-taught learning initializes the | |
939 model in the basin of attraction of supervised gradient descent | |
940 that corresponds to better generalization. Furthermore, such good | |
941 basins of attraction are not discovered by pure supervised learning | |
942 (with or without self-taught settings), and more labeled examples | |
550
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943 does not allow the model to go from the poorer basins of attraction discovered |
529 | 944 by the purely supervised shallow models to the kind of better basins associated |
945 with deep learning and self-taught learning. | |
502
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946 |
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947 A Flash demo of the recognizer (where both the MLP and the SDA can be compared) |
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948 can be executed on-line at {\tt http://deep.host22.com}. |
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949 |
498
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950 \newpage |
496
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951 { |
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952 \bibliography{strings,strings-short,strings-shorter,ift6266_ml,aigaion-shorter,specials} |
469 | 953 %\bibliographystyle{plainnat} |
954 \bibliographystyle{unsrtnat} | |
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955 %\bibliographystyle{apalike} |
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956 } |
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957 |
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958 |
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959 \end{document} |