Mercurial > ift6266
annotate writeup/nips2010_submission.tex @ 550:662299f265ab
suggestions from Ian
author | Yoshua Bengio <bengioy@iro.umontreal.ca> |
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date | Wed, 02 Jun 2010 15:44:46 -0400 |
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1 \documentclass{article} % For LaTeX2e |
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2 \usepackage{nips10submit_e,times} |
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3 |
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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} |
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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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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 |
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30 examples} and show that {\em deep learners benefit more from them than a |
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31 corresponding shallow learner}, in the area |
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32 of handwritten character recognition. In fact, we show that they reach |
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33 human-level performance on both handwritten digit classification and |
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34 62-class handwritten character recognition. For this purpose we |
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35 developed a powerful generator of stochastic variations and noise |
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36 processes for character images, including not only affine transformations but |
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37 also slant, local elastic deformations, changes in thickness, background |
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38 images, grey level changes, contrast, occlusion, and various types of |
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39 noise. The out-of-distribution examples are |
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40 obtained from these highly distorted images or |
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41 by including examples of object classes different from those in the target test set. |
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42 \end{abstract} |
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43 \vspace*{-2mm} |
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44 |
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45 \section{Introduction} |
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46 \vspace*{-1mm} |
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47 |
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48 Deep Learning has emerged as a promising new area of research in |
469 | 49 statistical machine learning (see~\citet{Bengio-2009} for a review). |
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50 Learning algorithms for deep architectures are centered on the learning |
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51 of useful representations of data, which are better suited to the task at hand. |
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52 This is in great part inspired by observations of the mammalian visual cortex, |
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53 which consists of a chain of processing elements, each of which is associated with a |
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54 different representation of the raw visual input. In fact, |
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55 it was found recently that the features learnt in deep architectures resemble |
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56 those observed in the first two of these stages (in areas V1 and V2 |
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57 of visual cortex)~\citep{HonglakL2008}, and that they become more and |
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58 more invariant to factors of variation (such as camera movement) in |
501 | 59 higher layers~\citep{Goodfellow2009}. |
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60 Learning a hierarchy of features increases the |
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61 ease and practicality of developing representations that are at once |
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62 tailored to specific tasks, yet are able to borrow statistical strength |
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63 from other related tasks (e.g., modeling different kinds of objects). Finally, learning the |
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64 feature representation can lead to higher-level (more abstract, more |
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65 general) features that are more robust to unanticipated sources of |
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66 variance extant in real data. |
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67 |
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68 Whereas a deep architecture can in principle be more powerful than a |
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69 shallow one in terms of representation, depth appears to render the |
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70 training problem more difficult in terms of optimization and local minima. |
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71 It is also only recently that successful algorithms were proposed to |
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72 overcome some of these difficulties. All are based on unsupervised |
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73 learning, often in an greedy layer-wise ``unsupervised pre-training'' |
469 | 74 stage~\citep{Bengio-2009}. One of these layer initialization techniques, |
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75 applied here, is the Denoising |
547 | 76 Auto-encoder~(DA)~\citep{VincentPLarochelleH2008-very-small} (see Figure~\ref{fig:da}), |
77 which | |
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78 performed similarly or better than previously proposed Restricted Boltzmann |
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79 Machines in terms of unsupervised extraction of a hierarchy of features |
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80 useful for classification. The principle is that each layer starting from |
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81 the bottom is trained to encode its input (the output of the previous |
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82 layer) and to reconstruct it from a corrupted version. After this |
547 | 83 unsupervised initialization, the stack of DAs can be |
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84 converted into a deep supervised feedforward neural network and fine-tuned by |
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85 stochastic gradient descent. |
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86 |
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87 Self-taught learning~\citep{RainaR2007} is a paradigm that combines principles |
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88 of semi-supervised and multi-task learning: the learner can exploit examples |
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89 that are unlabeled and/or come from a distribution different from the target |
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90 distribution, e.g., from other classes than those of interest. |
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91 It has already been shown that deep learners can clearly take advantage of |
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92 unsupervised learning and unlabeled examples~\citep{Bengio-2009,WestonJ2008-small}, |
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93 but more needs to be done to explore the impact |
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94 of {\em out-of-distribution} examples and of the multi-task setting |
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95 (one exception is~\citep{CollobertR2008}, which uses very different kinds |
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96 of learning algorithms). In particular the {\em relative |
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97 advantage} of deep learning for these settings has not been evaluated. |
512 | 98 The hypothesis explored here is that a deep hierarchy of features |
99 may be better able to provide sharing of statistical strength | |
100 between different regions in input space or different tasks, | |
101 as discussed in the conclusion. | |
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102 |
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103 In this paper we ask the following questions: |
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104 |
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105 %\begin{enumerate} |
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106 $\bullet$ %\item |
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107 Do the good results previously obtained with deep architectures on the |
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108 MNIST digit images generalize to the setting of a much larger and richer (but similar) |
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109 dataset, the NIST special database 19, with 62 classes and around 800k examples? |
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110 |
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111 $\bullet$ %\item |
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112 To what extent does the perturbation of input images (e.g. adding |
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113 noise, affine transformations, background images) make the resulting |
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114 classifiers better not only on similarly perturbed images but also on |
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115 the {\em original clean examples}? |
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116 |
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117 $\bullet$ %\item |
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118 Do deep architectures {\em benefit more from such out-of-distribution} |
469 | 119 examples, i.e. do they benefit more from the self-taught learning~\citep{RainaR2007} framework? |
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120 |
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121 $\bullet$ %\item |
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122 Similarly, does the feature learning step in deep learning algorithms benefit more |
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123 from training with moderately different classes (i.e. a multi-task learning scenario) than |
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124 a corresponding shallow and purely supervised architecture? |
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125 %\end{enumerate} |
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126 |
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127 Our experimental results provide positive evidence towards all of these questions. |
547 | 128 To achieve these results, we introduce in the next section a sophisticated system |
129 for stochastically transforming character images. The conclusion discusses | |
130 the more general question of why deep learners may benefit so much from | |
131 the self-taught learning framework. | |
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132 |
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133 \vspace*{-1mm} |
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134 \section{Perturbation and Transformation of Character Images} |
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135 \label{s:perturbations} |
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136 \vspace*{-1mm} |
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137 |
467 | 138 This section describes the different transformations we used to stochastically |
547 | 139 transform source images in order to obtain data from a larger distribution which |
140 covers a domain substantially larger than the clean characters distribution from | |
141 which we start. Although character transformations have been used before to | |
142 improve character recognizers, this effort is on a large scale both | |
143 in number of classes and in the complexity of the transformations, hence | |
144 in the complexity of the learning task. | |
145 More details can | |
469 | 146 be found in this technical report~\citep{ift6266-tr-anonymous}. |
464
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147 The code for these transformations (mostly python) is available at |
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148 {\tt http://anonymous.url.net}. All the modules in the pipeline share |
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149 a global control parameter ($0 \le complexity \le 1$) that allows one to modulate the |
467 | 150 amount of deformation or noise introduced. |
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151 |
467 | 152 There are two main parts in the pipeline. The first one, |
153 from slant to pinch below, performs transformations. The second | |
154 part, from blur to contrast, adds different kinds of noise. | |
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155 |
523 | 156 \begin{figure}[ht] |
541 | 157 \vspace*{-2mm} |
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158 \centerline{\resizebox{.9\textwidth}{!}{\includegraphics{images/transfo.png}}} |
506 | 159 % TODO: METTRE LE NOM DE LA TRANSFO A COTE DE CHAQUE IMAGE |
501 | 160 \caption{Illustration of each transformation applied alone to the same image |
161 of an upper-case h (top left). First row (from left to right) : original image, slant, | |
162 thickness, affine transformation (translation, rotation, shear), | |
163 local elastic deformation; second row (from left to right) : | |
164 pinch, motion blur, occlusion, pixel permutation, Gaussian noise; third row (from left to right) : | |
165 background image, salt and pepper noise, spatially Gaussian noise, scratches, | |
166 grey level and contrast changes.} | |
167 \label{fig:transfo} | |
541 | 168 \vspace*{-2mm} |
501 | 169 \end{figure} |
170 | |
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171 {\large\bf Transformations} |
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172 |
541 | 173 \vspace*{0.5mm} |
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174 |
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175 {\bf Slant.} |
541 | 176 Each row of the image is shifted |
495 | 177 proportionally to its height: $shift = round(slant \times height)$. |
541 | 178 $slant \sim U[-complexity,complexity]$. |
179 \vspace*{-1mm} | |
523 | 180 |
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181 {\bf Thickness.} |
495 | 182 Morphological operators of dilation and erosion~\citep{Haralick87,Serra82} |
467 | 183 are applied. The neighborhood of each pixel is multiplied |
184 element-wise with a {\em structuring element} matrix. | |
185 The pixel value is replaced by the maximum or the minimum of the resulting | |
186 matrix, respectively for dilation or erosion. Ten different structural elements with | |
187 increasing dimensions (largest is $5\times5$) were used. For each image, | |
188 randomly sample the operator type (dilation or erosion) with equal probability and one structural | |
541 | 189 element from a subset of the $n=round(m \times complexity)$ smallest structuring elements |
190 where $m=10$ for dilation and $m=6$ for erosion (to avoid completely erasing thin characters). | |
191 A neutral element (no transformation) | |
192 is always present in the set. is applied. | |
193 \vspace*{-1mm} | |
523 | 194 |
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195 {\bf Affine Transformations.} |
467 | 196 A $2 \times 3$ affine transform matrix (with |
197 6 parameters $(a,b,c,d,e,f)$) is sampled according to the $complexity$ level. | |
541 | 198 Output pixel $(x,y)$ takes the value of input pixel |
199 nearest to $(ax+by+c,dx+ey+f)$, | |
200 producing scaling, translation, rotation and shearing. | |
467 | 201 The marginal distributions of $(a,b,c,d,e,f)$ have been tuned by hand to |
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202 forbid large rotations (not to confuse classes) but to give good |
467 | 203 variability of the transformation: $a$ and $d$ $\sim U[1-3 \times |
204 complexity,1+3 \times complexity]$, $b$ and $e$ $\sim[-3 \times complexity,3 | |
205 \times complexity]$ and $c$ and $f$ $\sim U[-4 \times complexity, 4 \times | |
523 | 206 complexity]$. |
541 | 207 \vspace*{-1mm} |
523 | 208 |
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209 {\bf Local Elastic Deformations.} |
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210 This filter induces a ``wiggly'' effect in the image, following~\citet{SimardSP03-short}, |
467 | 211 which provides more details. |
541 | 212 The intensity of the displacement fields is given by |
213 $\alpha = \sqrt[3]{complexity} \times 10.0$, which are | |
214 convolved with a Gaussian 2D kernel (resulting in a blur) of | |
215 standard deviation $\sigma = 10 - 7 \times\sqrt[3]{complexity}$. | |
216 \vspace*{-1mm} | |
523 | 217 |
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218 {\bf Pinch.} |
541 | 219 This is the ``Whirl and pinch'' GIMP filter but with whirl was set to 0. |
220 A pinch is ``similar to projecting the image onto an elastic | |
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221 surface and pressing or pulling on the center of the surface'' (GIMP documentation manual). |
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222 For a square input image, this is akin to drawing a circle of |
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223 radius $r$ around a center point $C$. Any point (pixel) $P$ belonging to |
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224 that disk (region inside circle) will have its value recalculated by taking |
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225 the value of another ``source'' pixel in the original image. The position of |
495 | 226 that source pixel is found on the line that goes through $C$ and $P$, but |
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227 at some other distance $d_2$. Define $d_1$ to be the distance between $P$ |
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228 and $C$. $d_2$ is given by $d_2 = sin(\frac{\pi{}d_1}{2r})^{-pinch} \times |
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229 d_1$, where $pinch$ is a parameter to the filter. |
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230 The actual value is given by bilinear interpolation considering the pixels |
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231 around the (non-integer) source position thus found. |
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232 Here $pinch \sim U[-complexity, 0.7 \times complexity]$. |
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233 |
541 | 234 \vspace*{0.5mm} |
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235 |
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236 {\large\bf Injecting Noise} |
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237 |
541 | 238 \vspace*{0.5mm} |
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239 |
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240 {\bf Motion Blur.} |
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241 This is GIMP's ``linear motion blur'' |
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242 with parameters $length$ and $angle$. The value of |
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243 a pixel in the final image is approximately the mean value of the first $length$ pixels |
467 | 244 found by moving in the $angle$ direction. |
523 | 245 Here $angle \sim U[0,360]$ degrees, and $length \sim {\rm Normal}(0,(3 \times complexity)^2)$. |
541 | 246 \vspace*{-1mm} |
523 | 247 |
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248 {\bf Occlusion.} |
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249 Selects a random rectangle from an {\em occluder} character |
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250 image and places it over the original {\em occluded} |
467 | 251 image. Pixels are combined by taking the max(occluder,occluded), |
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252 closer to black. The rectangle corners |
467 | 253 are sampled so that larger complexity gives larger rectangles. |
254 The destination position in the occluded image are also sampled | |
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255 according to a normal distribution (more details in~\citet{ift6266-tr-anonymous}). |
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256 This filter is skipped with probability 60\%. |
541 | 257 \vspace*{-1mm} |
523 | 258 |
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259 {\bf Pixel Permutation.} |
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260 This filter permutes neighbouring pixels. It first selects |
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261 fraction $\frac{complexity}{3}$ of pixels randomly in the image. Each of them are then |
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262 sequentially exchanged with one other in as $V4$ neighbourhood. |
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263 This filter is skipped with probability 80\%. |
541 | 264 \vspace*{-1mm} |
523 | 265 |
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266 {\bf Gaussian Noise.} |
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267 This filter simply adds, to each pixel of the image independently, a |
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268 noise $\sim Normal(0,(\frac{complexity}{10})^2)$. |
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269 This filter is skipped with probability 70\%. |
541 | 270 \vspace*{-1mm} |
523 | 271 |
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272 {\bf Background Images.} |
469 | 273 Following~\citet{Larochelle-jmlr-2009}, this transformation adds a random |
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274 background behind the letter, from a randomly chosen natural image, |
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275 with contrast adjustments depending on $complexity$, to preserve |
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276 more or less of the original character image. |
541 | 277 \vspace*{-1mm} |
523 | 278 |
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279 {\bf Salt and Pepper Noise.} |
467 | 280 This filter adds noise $\sim U[0,1]$ to random subsets of pixels. |
281 The number of selected pixels is $0.2 \times complexity$. | |
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282 This filter is skipped with probability 75\%. |
541 | 283 \vspace*{-1mm} |
523 | 284 |
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285 {\bf Spatially Gaussian Noise.} |
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286 Different regions of the image are spatially smoothed by convolving |
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287 the image is convolved with a symmetric Gaussian kernel of |
495 | 288 size and variance chosen uniformly in the ranges $[12,12 + 20 \times |
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289 complexity]$ and $[2,2 + 6 \times complexity]$. The result is normalized |
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290 between $0$ and $1$. We also create a symmetric averaging window, of the |
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291 kernel size, with maximum value at the center. For each image we sample |
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292 uniformly from $3$ to $3 + 10 \times complexity$ pixels that will be |
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293 averaging centers between the original image and the filtered one. We |
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294 initialize to zero a mask matrix of the image size. For each selected pixel |
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295 we add to the mask the averaging window centered to it. The final image is |
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296 computed from the following element-wise operation: $\frac{image + filtered |
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297 image \times mask}{mask+1}$. |
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298 This filter is skipped with probability 75\%. |
541 | 299 \vspace*{-1mm} |
523 | 300 |
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301 {\bf Scratches.} |
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302 The scratches module places line-like white patches on the image. The |
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303 lines are heavily transformed images of the digit ``1'' (one), chosen |
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304 at random among 500 such 1 images, |
467 | 305 randomly cropped and rotated by an angle $\sim Normal(0,(100 \times |
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306 complexity)^2$, using bi-cubic interpolation. |
495 | 307 Two passes of a grey-scale morphological erosion filter |
467 | 308 are applied, reducing the width of the line |
309 by an amount controlled by $complexity$. | |
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310 This filter is skipped with probability 85\%. The probabilities |
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311 of applying 1, 2, or 3 patches are (50\%,30\%,20\%). |
541 | 312 \vspace*{-1mm} |
523 | 313 |
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314 {\bf Grey Level and Contrast Changes.} |
495 | 315 This filter changes the contrast and may invert the image polarity (white |
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316 to black and black to white). The contrast is $C \sim U[1-0.85 \times complexity,1]$ |
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317 so the image is normalized into $[\frac{1-C}{2},1-\frac{1-C}{2}]$. The |
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318 polarity is inverted with probability 50\%. |
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319 |
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320 \iffalse |
523 | 321 \begin{figure}[ht] |
538 | 322 \centerline{\resizebox{.9\textwidth}{!}{\includegraphics{images/example_t.png}}}\\ |
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323 \caption{Illustration of the pipeline of stochastic |
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324 transformations applied to the image of a lower-case \emph{t} |
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325 (the upper left image). Each image in the pipeline (going from |
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326 left to right, first top line, then bottom line) shows the result |
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327 of applying one of the modules in the pipeline. The last image |
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328 (bottom right) is used as training example.} |
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329 \label{fig:pipeline} |
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330 \end{figure} |
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331 \fi |
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332 |
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333 |
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334 \vspace*{-1mm} |
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335 \section{Experimental Setup} |
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336 \vspace*{-1mm} |
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337 |
472 | 338 Whereas much previous work on deep learning algorithms had been performed on |
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339 the MNIST digits classification task~\citep{Hinton06,ranzato-07-small,Bengio-nips-2006,Salakhutdinov+Hinton-2009}, |
472 | 340 with 60~000 examples, and variants involving 10~000 |
501 | 341 examples~\citep{Larochelle-jmlr-toappear-2008,VincentPLarochelleH2008}, we want |
472 | 342 to focus here on the case of much larger training sets, from 10 times to |
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343 to 1000 times larger. |
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344 |
535 | 345 The first step in constructing the larger datasets (called NISTP and P07) is to sample from |
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346 a {\em data source}: {\bf NIST} (NIST database 19), {\bf Fonts}, {\bf Captchas}, |
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347 and {\bf OCR data} (scanned machine printed characters). Once a character |
547 | 348 is sampled from one of these sources (chosen randomly), the second step is to |
349 apply a pipeline of transformations and/or noise processes described in section \ref{s:perturbations}. | |
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350 |
547 | 351 To provide a baseline of error rate comparison we also estimate human performance |
352 on both the 62-class task and the 10-class digits task. | |
535 | 353 We compare the best MLPs against |
354 the best SDAs (both models' hyper-parameters are selected to minimize the validation set error), | |
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355 along with a comparison against a precise estimate |
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356 of human performance obtained via Amazon's Mechanical Turk (AMT) |
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357 service (http://mturk.com). |
502
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358 AMT users are paid small amounts |
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359 of money to perform tasks for which human intelligence is required. |
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360 Mechanical Turk has been used extensively in natural language processing and vision. |
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361 %processing \citep{SnowEtAl2008} and vision |
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362 %\citep{SorokinAndForsyth2008,whitehill09}. |
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363 AMT users were presented |
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364 with 10 character images and asked to choose 10 corresponding ASCII |
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365 characters. They were forced to make a hard choice among the |
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366 62 or 10 character classes (all classes or digits only). |
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367 A total 2500 images/dataset were classified by XXX subjects, |
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368 with 3 subjects classifying each image, allowing |
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369 us to estimate inter-human variability (e.g a standard error of 0.1\% |
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370 on the average 18\% error done by humans on the 62-class task). |
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371 |
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372 \vspace*{-1mm} |
472 | 373 \subsection{Data Sources} |
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374 \vspace*{-1mm} |
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375 |
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376 %\begin{itemize} |
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377 %\item |
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378 {\bf NIST.} |
501 | 379 Our main source of characters is the NIST Special Database 19~\citep{Grother-1995}, |
472 | 380 widely used for training and testing character |
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381 recognition systems~\citep{Granger+al-2007,Cortes+al-2000,Oliveira+al-2002-short,Milgram+al-2005}. |
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382 The dataset is composed of 814255 digits and characters (upper and lower cases), with hand checked classifications, |
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383 extracted from handwritten sample forms of 3600 writers. The characters are labelled by one of the 62 classes |
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384 corresponding to ``0''-``9'',``A''-``Z'' and ``a''-``z''. The dataset contains 8 parts (partitions) of varying complexity. |
534 | 385 The fourth partition (called $hsf_4$, 82587 examples), |
386 experimentally recognized to be the most difficult one, is the one recommended | |
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387 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 | 388 for that purpose. We randomly split the remainder (731668 examples) into a training set and a validation set for |
389 model selection. | |
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390 The performances reported by previous work on that dataset mostly use only the digits. |
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391 Here we use all the classes both in the training and testing phase. This is especially |
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392 useful to estimate the effect of a multi-task setting. |
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393 Note that the distribution of the classes in the NIST training and test sets differs |
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394 substantially, with relatively many more digits in the test set, and more uniform distribution |
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395 of letters in the test set, compared to the training set (in the latter, the letters are distributed |
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396 more like the natural distribution of letters in text). |
549 | 397 \vspace*{-1mm} |
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398 |
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399 %\item |
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400 {\bf Fonts.} |
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401 In order to have a good variety of sources we downloaded an important number of free fonts from: |
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402 {\tt http://cg.scs.carleton.ca/\textasciitilde luc/freefonts.html}. |
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403 % TODO: pointless to anonymize, it's not pointing to our work |
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404 Including the operating system's (Windows 7) fonts, there is a total of $9817$ different fonts that we can choose uniformly from. |
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405 The chosen {\tt ttf} file is either used as input of the Captcha generator (see next item) or, by producing a corresponding image, |
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406 directly as input to our models. |
549 | 407 \vspace*{-1mm} |
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408 |
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409 %\item |
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410 {\bf Captchas.} |
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411 The Captcha data source is an adaptation of the \emph{pycaptcha} library (a python based captcha generator library) for |
472 | 412 generating characters of the same format as the NIST dataset. This software is based on |
495 | 413 a random character class generator and various kinds of transformations similar to those described in the previous sections. |
472 | 414 In order to increase the variability of the data generated, many different fonts are used for generating the characters. |
495 | 415 Transformations (slant, distortions, rotation, translation) are applied to each randomly generated character with a complexity |
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416 depending on the value of the complexity parameter provided by the user of the data source. |
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417 %Two levels of complexity are allowed and can be controlled via an easy to use facade class. %TODO: what's a facade class? |
549 | 418 \vspace*{-1mm} |
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419 |
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420 %\item |
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421 {\bf OCR data.} |
472 | 422 A large set (2 million) of scanned, OCRed and manually verified machine-printed |
423 characters (from various documents and books) where included as an | |
424 additional source. This set is part of a larger corpus being collected by the Image Understanding | |
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425 Pattern Recognition Research group led by Thomas Breuel at University of Kaiserslautern |
495 | 426 ({\tt http://www.iupr.com}), and which will be publicly released. |
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427 %TODO: let's hope that Thomas is not a reviewer! :) Seriously though, maybe we should anonymize this |
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428 %\end{itemize} |
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429 |
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430 \vspace*{-1mm} |
472 | 431 \subsection{Data Sets} |
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432 \vspace*{-1mm} |
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433 |
472 | 434 All data sets contain 32$\times$32 grey-level images (values in $[0,1]$) associated with a label |
435 from one of the 62 character classes. | |
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436 %\begin{itemize} |
549 | 437 \vspace*{-1mm} |
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438 |
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439 %\item |
534 | 440 {\bf NIST.} This is the raw NIST special database 19~\citep{Grother-1995}. It has |
535 | 441 \{651668 / 80000 / 82587\} \{training / validation / test\} examples. |
549 | 442 \vspace*{-1mm} |
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443 |
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444 %\item |
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445 {\bf P07.} This dataset is obtained by taking raw characters from all four of the above sources |
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446 and sending them through the transformation pipeline described in section \ref{s:perturbations}. |
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447 For each new example to generate, a data source is selected with probability $10\%$ from the fonts, |
472 | 448 $25\%$ from the captchas, $25\%$ from the OCR data and $40\%$ from NIST. We apply all the transformations in the |
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449 order given above, and for each of them we sample uniformly a \emph{complexity} in the range $[0,0.7]$. |
535 | 450 It has \{81920000 / 80000 / 20000\} \{training / validation / test\} examples. |
549 | 451 \vspace*{-1mm} |
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452 |
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453 %\item |
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454 {\bf NISTP.} This one is equivalent to P07 (complexity parameter of $0.7$ with the same proportions of data sources) |
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455 except that we only apply |
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456 transformations from slant to pinch. Therefore, the character is |
495 | 457 transformed but no additional noise is added to the image, giving images |
534 | 458 closer to the NIST dataset. |
535 | 459 It has \{81920000 / 80000 / 20000\} \{training / validation / test\} examples. |
484
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460 %\end{itemize} |
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461 |
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462 \vspace*{-1mm} |
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463 \subsection{Models and their Hyperparameters} |
484
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464 \vspace*{-1mm} |
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465 |
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466 The experiments are performed with Multi-Layer Perceptrons (MLP) with a single |
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467 hidden layer and with Stacked Denoising Auto-Encoders (SDA). |
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468 \emph{Note that all hyper-parameters are selected based on performance on the {\bf NISTP} validation set.} |
472 | 469 |
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470 {\bf Multi-Layer Perceptrons (MLP).} |
472 | 471 Whereas previous work had compared deep architectures to both shallow MLPs and |
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472 SVMs, we only compared to MLPs here because of the very large datasets used |
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473 (making the use of SVMs computationally challenging because of their quadratic |
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474 scaling behavior). |
472 | 475 The MLP has a single hidden layer with $\tanh$ activation functions, and softmax (normalized |
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476 exponentials) on the output layer for estimating $P(class | image)$. |
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477 The number of hidden units is taken in $\{300,500,800,1000,1500\}$. |
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478 Training examples are presented in minibatches of size 20. A constant learning |
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479 rate was chosen among $\{0.001, 0.01, 0.025, 0.075, 0.1, 0.5\}$ |
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480 through preliminary experiments (measuring performance on a validation set), |
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481 and $0.1$ was then selected for optimizing on the whole training sets. |
549 | 482 \vspace*{-1mm} |
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483 |
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484 |
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485 {\bf Stacked Denoising Auto-Encoders (SDA).} |
472 | 486 Various auto-encoder variants and Restricted Boltzmann Machines (RBMs) |
487 can be used to initialize the weights of each layer of a deep MLP (with many hidden | |
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488 layers)~\citep{Hinton06,ranzato-07-small,Bengio-nips-2006}, |
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489 apparently setting parameters in the |
472 | 490 basin of attraction of supervised gradient descent yielding better |
491 generalization~\citep{Erhan+al-2010}. It is hypothesized that the | |
492 advantage brought by this procedure stems from a better prior, | |
493 on the one hand taking advantage of the link between the input | |
494 distribution $P(x)$ and the conditional distribution of interest | |
495 $P(y|x)$ (like in semi-supervised learning), and on the other hand | |
496 taking advantage of the expressive power and bias implicit in the | |
497 deep architecture (whereby complex concepts are expressed as | |
498 compositions of simpler ones through a deep hierarchy). | |
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499 |
547 | 500 \begin{figure}[ht] |
501 \vspace*{-2mm} | |
502 \centerline{\resizebox{0.8\textwidth}{!}{\includegraphics{images/denoising_autoencoder_small.pdf}}} | |
549 | 503 \vspace*{-2mm} |
547 | 504 \caption{Illustration of the computations and training criterion for the denoising |
505 auto-encoder used to pre-train each layer of the deep architecture. Input $x$ of | |
506 the layer (i.e. raw input or output of previous layer) | |
507 is corrupted into $\tilde{x}$ and encoded into code $y$ by the encoder $f_\theta(\cdot)$. | |
508 The decoder $g_{\theta'}(\cdot)$ maps $y$ to reconstruction $z$, which | |
509 is compared to the uncorrupted input $x$ through the loss function | |
510 $L_H(x,z)$, whose expected value is approximately minimized during training | |
511 by tuning $\theta$ and $\theta'$.} | |
512 \label{fig:da} | |
513 \vspace*{-2mm} | |
514 \end{figure} | |
515 | |
472 | 516 Here we chose to use the Denoising |
517 Auto-Encoder~\citep{VincentPLarochelleH2008} as the building block for | |
518 these deep hierarchies of features, as it is very simple to train and | |
532
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519 explain (see Figure~\ref{fig:da}, as well as |
521
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520 tutorial and code there: {\tt http://deeplearning.net/tutorial}), |
472 | 521 provides immediate and efficient inference, and yielded results |
522 comparable or better than RBMs in series of experiments | |
519
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523 \citep{VincentPLarochelleH2008}. During training, a Denoising |
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524 Auto-Encoder is presented with a stochastically corrupted version |
472 | 525 of the input and trained to reconstruct the uncorrupted input, |
526 forcing the hidden units to represent the leading regularities in | |
535 | 527 the data. Once it is trained, in a purely unsupervised way, |
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528 its hidden units' activations can |
472 | 529 be used as inputs for training a second one, etc. |
530 After this unsupervised pre-training stage, the parameters | |
531 are used to initialize a deep MLP, which is fine-tuned by | |
532 the same standard procedure used to train them (see previous section). | |
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533 The SDA hyper-parameters are the same as for the MLP, with the addition of the |
472 | 534 amount of corruption noise (we used the masking noise process, whereby a |
535 fixed proportion of the input values, randomly selected, are zeroed), and a | |
536 separate learning rate for the unsupervised pre-training stage (selected | |
537 from the same above set). The fraction of inputs corrupted was selected | |
538 among $\{10\%, 20\%, 50\%\}$. Another hyper-parameter is the number | |
539 of hidden layers but it was fixed to 3 based on previous work with | |
547 | 540 SDAs on MNIST~\citep{VincentPLarochelleH2008}. |
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541 |
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542 \vspace*{-1mm} |
523 | 543 |
544 \begin{figure}[ht] | |
541 | 545 \vspace*{-2mm} |
523 | 546 \centerline{\resizebox{.99\textwidth}{!}{\includegraphics{images/error_rates_charts.pdf}}} |
549 | 547 \vspace*{-3mm} |
547 | 548 \caption{SDAx are the {\bf deep} models. Error bars indicate a 95\% confidence interval. 0 indicates that the model was trained |
523 | 549 on NIST, 1 on NISTP, and 2 on P07. Left: overall results |
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550 of all models, on NIST and NISTP test sets. |
523 | 551 Right: error rates on NIST test digits only, along with the previous results from |
552 literature~\citep{Granger+al-2007,Cortes+al-2000,Oliveira+al-2002-short,Milgram+al-2005} | |
553 respectively based on ART, nearest neighbors, MLPs, and SVMs.} | |
554 \label{fig:error-rates-charts} | |
541 | 555 \vspace*{-2mm} |
523 | 556 \end{figure} |
557 | |
558 | |
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559 \section{Experimental Results} |
549 | 560 \vspace*{-2mm} |
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561 |
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562 %\vspace*{-1mm} |
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563 %\subsection{SDA vs MLP vs Humans} |
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564 %\vspace*{-1mm} |
535 | 565 The models are either trained on NIST (MLP0 and SDA0), |
566 NISTP (MLP1 and SDA1), or P07 (MLP2 and SDA2), and tested | |
550
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567 on either NIST, NISTP or P07, either on the 62-class task |
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568 or on the 10-digits task. |
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569 Figure~\ref{fig:error-rates-charts} summarizes the results obtained, |
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570 comparing humans, the three MLPs (MLP0, MLP1, MLP2) and the three SDAs (SDA0, SDA1, |
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571 SDA2), along with the previous results on the digits NIST special database |
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572 19 test set from the literature respectively based on ARTMAP neural |
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573 networks ~\citep{Granger+al-2007}, fast nearest-neighbor search |
516
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574 ~\citep{Cortes+al-2000}, MLPs ~\citep{Oliveira+al-2002-short}, and SVMs |
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575 ~\citep{Milgram+al-2005}. More detailed and complete numerical results |
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576 (figures and tables, including standard errors on the error rates) can be |
535 | 577 found in Appendix I of the supplementary material. |
578 The deep learner not only outperformed the shallow ones and | |
493
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579 previously published performance (in a statistically and qualitatively |
535 | 580 significant way) but when trained with perturbed data |
581 reaches human performance on both the 62-class task | |
523 | 582 and the 10-class (digits) task. |
550
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583 17\% error (SDA1) or 18\% error (humans) may seem large but a large |
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584 majority of the errors from humans and from SDA1 are from out-of-context |
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585 confusions (e.g. a vertical bar can be a ``1'', an ``l'' or an ``L'', and a |
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586 ``c'' and a ``C'' are often indistinguishible). |
523 | 587 |
588 \begin{figure}[ht] | |
549 | 589 \vspace*{-3mm} |
523 | 590 \centerline{\resizebox{.99\textwidth}{!}{\includegraphics{images/improvements_charts.pdf}}} |
549 | 591 \vspace*{-3mm} |
523 | 592 \caption{Relative improvement in error rate due to self-taught learning. |
593 Left: Improvement (or loss, when negative) | |
594 induced by out-of-distribution examples (perturbed data). | |
595 Right: Improvement (or loss, when negative) induced by multi-task | |
596 learning (training on all classes and testing only on either digits, | |
597 upper case, or lower-case). The deep learner (SDA) benefits more from | |
598 both self-taught learning scenarios, compared to the shallow MLP.} | |
599 \label{fig:improvements-charts} | |
600 \vspace*{-2mm} | |
601 \end{figure} | |
602 | |
603 In addition, as shown in the left of | |
604 Figure~\ref{fig:improvements-charts}, the relative improvement in error | |
493
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605 rate brought by self-taught learning is greater for the SDA, and these |
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606 differences with the MLP are statistically and qualitatively |
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607 significant. |
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608 The left side of the figure shows the improvement to the clean |
493
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609 NIST test set error brought by the use of out-of-distribution examples |
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610 (i.e. the perturbed examples examples from NISTP or P07). |
547 | 611 Relative percent change is measured by taking |
548
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612 $100 \% \times$ (original model's error / perturbed-data model's error - 1). |
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613 The right side of |
523 | 614 Figure~\ref{fig:improvements-charts} shows the relative improvement |
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615 brought by the use of a multi-task setting, in which the same model is |
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616 trained for more classes than the target classes of interest (i.e. training |
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617 with all 62 classes when the target classes are respectively the digits, |
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618 lower-case, or upper-case characters). Again, whereas the gain from the |
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619 multi-task setting is marginal or negative for the MLP, it is substantial |
547 | 620 for the SDA. Note that to simplify these multi-task experiments, only the original |
493
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621 NIST dataset is used. For example, the MLP-digits bar shows the relative |
547 | 622 percent improvement in MLP error rate on the NIST digits test set |
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623 is $100\% \times$ (1 - single-task |
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624 model's error / multi-task model's error). The single-task model is |
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625 trained with only 10 outputs (one per digit), seeing only digit examples, |
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626 whereas the multi-task model is trained with 62 outputs, with all 62 |
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627 character classes as examples. Hence the hidden units are shared across |
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628 all tasks. For the multi-task model, the digit error rate is measured by |
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629 comparing the correct digit class with the output class associated with the |
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630 maximum conditional probability among only the digit classes outputs. The |
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631 setting is similar for the other two target classes (lower case characters |
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632 and upper case characters). |
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633 %\vspace*{-1mm} |
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634 %\subsection{Perturbed Training Data More Helpful for SDA} |
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635 %\vspace*{-1mm} |
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636 |
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637 %\vspace*{-1mm} |
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638 %\subsection{Multi-Task Learning Effects} |
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639 %\vspace*{-1mm} |
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640 |
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641 \iffalse |
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642 As previously seen, the SDA is better able to benefit from the |
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643 transformations applied to the data than the MLP. In this experiment we |
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644 define three tasks: recognizing digits (knowing that the input is a digit), |
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645 recognizing upper case characters (knowing that the input is one), and |
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646 recognizing lower case characters (knowing that the input is one). We |
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647 consider the digit classification task as the target task and we want to |
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648 evaluate whether training with the other tasks can help or hurt, and |
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649 whether the effect is different for MLPs versus SDAs. The goal is to find |
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650 out if deep learning can benefit more (or less) from multiple related tasks |
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651 (i.e. the multi-task setting) compared to a corresponding purely supervised |
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652 shallow learner. |
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653 |
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654 We use a single hidden layer MLP with 1000 hidden units, and a SDA |
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655 with 3 hidden layers (1000 hidden units per layer), pre-trained and |
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656 fine-tuned on NIST. |
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657 |
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658 Our results show that the MLP benefits marginally from the multi-task setting |
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659 in the case of digits (5\% relative improvement) but is actually hurt in the case |
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660 of characters (respectively 3\% and 4\% worse for lower and upper class characters). |
495 | 661 On the other hand the SDA benefited from the multi-task setting, with relative |
464
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662 error rate improvements of 27\%, 15\% and 13\% respectively for digits, |
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663 lower and upper case characters, as shown in Table~\ref{tab:multi-task}. |
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664 \fi |
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665 |
475 | 666 |
549 | 667 \vspace*{-2mm} |
529 | 668 \section{Conclusions and Discussion} |
549 | 669 \vspace*{-2mm} |
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670 |
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671 We have found that the self-taught learning framework is more beneficial |
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672 to a deep learner than to a traditional shallow and purely |
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673 supervised learner. More precisely, |
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674 the answers are positive for all the questions asked in the introduction. |
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675 %\begin{itemize} |
487 | 676 |
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677 $\bullet$ %\item |
547 | 678 {\bf Do the good results previously obtained with deep architectures on the |
549 | 679 MNIST digits generalize to a much larger and richer (but similar) |
547 | 680 dataset, the NIST special database 19, with 62 classes and around 800k examples}? |
502
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681 Yes, the SDA {\bf systematically outperformed the MLP and all the previously |
529 | 682 published results on this dataset} (the ones that we are aware of), {\bf in fact reaching human-level |
683 performance} at around 17\% error on the 62-class task and 1.4\% on the digits. | |
484
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684 |
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685 $\bullet$ %\item |
547 | 686 {\bf To what extent do self-taught learning scenarios help deep learners, |
687 and do they help them more than shallow supervised ones}? | |
529 | 688 We found that distorted training examples not only made the resulting |
689 classifier better on similarly perturbed images but also on | |
690 the {\em original clean examples}, and more importantly and more novel, | |
691 that deep architectures benefit more from such {\em out-of-distribution} | |
692 examples. MLPs were helped by perturbed training examples when tested on perturbed input | |
502
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693 images (65\% relative improvement on NISTP) |
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694 but only marginally helped (5\% relative improvement on all classes) |
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695 or even hurt (10\% relative loss on digits) |
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696 with respect to clean examples . On the other hand, the deep SDAs |
472 | 697 were very significantly boosted by these out-of-distribution examples. |
529 | 698 Similarly, whereas the improvement due to the multi-task setting was marginal or |
502
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699 negative for the MLP (from +5.6\% to -3.6\% relative change), |
547 | 700 it was very significant for the SDA (from +13\% to +27\% relative change), |
701 which may be explained by the arguments below. | |
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702 %\end{itemize} |
472 | 703 |
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704 In the original self-taught learning framework~\citep{RainaR2007}, the |
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705 out-of-sample examples were used as a source of unsupervised data, and |
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706 experiments showed its positive effects in a \emph{limited labeled data} |
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707 scenario. However, many of the results by \citet{RainaR2007} (who used a |
550
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708 shallow, sparse coding approach) suggest that the {\em relative gain of self-taught |
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709 learning vs ordinary supervised learning} diminishes as the number of labeled examples increases. |
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710 We note instead that, for deep |
524
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711 architectures, our experiments show that such a positive effect is accomplished |
550
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712 even in a scenario with a \emph{very large number of labeled examples}, |
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713 i.e., here, the relative gain of self-taught learning is probably preserved |
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714 in the asymptotic regime. |
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715 |
547 | 716 {\bf Why would deep learners benefit more from the self-taught learning framework}? |
502
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717 The key idea is that the lower layers of the predictor compute a hierarchy |
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718 of features that can be shared across tasks or across variants of the |
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719 input distribution. Intermediate features that can be used in different |
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720 contexts can be estimated in a way that allows to share statistical |
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721 strength. Features extracted through many levels are more likely to |
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722 be more abstract (as the experiments in~\citet{Goodfellow2009} suggest), |
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723 increasing the likelihood that they would be useful for a larger array |
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724 of tasks and input conditions. |
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725 Therefore, we hypothesize that both depth and unsupervised |
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726 pre-training play a part in explaining the advantages observed here, and future |
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727 experiments could attempt at teasing apart these factors. |
529 | 728 And why would deep learners benefit from the self-taught learning |
729 scenarios even when the number of labeled examples is very large? | |
730 We hypothesize that this is related to the hypotheses studied | |
731 in~\citet{Erhan+al-2010}. Whereas in~\citet{Erhan+al-2010} | |
732 it was found that online learning on a huge dataset did not make the | |
733 advantage of the deep learning bias vanish, a similar phenomenon | |
734 may be happening here. We hypothesize that unsupervised pre-training | |
735 of a deep hierarchy with self-taught learning initializes the | |
736 model in the basin of attraction of supervised gradient descent | |
737 that corresponds to better generalization. Furthermore, such good | |
738 basins of attraction are not discovered by pure supervised learning | |
739 (with or without self-taught settings), and more labeled examples | |
550
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740 does not allow the model to go from the poorer basins of attraction discovered |
529 | 741 by the purely supervised shallow models to the kind of better basins associated |
742 with deep learning and self-taught learning. | |
502
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743 |
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744 A Flash demo of the recognizer (where both the MLP and the SDA can be compared) |
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745 can be executed on-line at {\tt http://deep.host22.com}. |
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746 |
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747 \newpage |
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748 { |
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749 \bibliography{strings,strings-short,strings-shorter,ift6266_ml,aigaion-shorter,specials} |
469 | 750 %\bibliographystyle{plainnat} |
751 \bibliographystyle{unsrtnat} | |
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752 %\bibliographystyle{apalike} |
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753 } |
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754 |
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755 |
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756 \end{document} |