annotate writeup/techreport.tex @ 562:3a4d4143434d

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author Frederic Bastien <nouiz@nouiz.org>
date Thu, 03 Jun 2010 12:59:11 -0400
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1 \documentclass[12pt,letterpaper]{article}
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2 \usepackage[utf8]{inputenc}
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3 \usepackage{graphicx}
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4 \usepackage{times}
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5 \usepackage{mlapa}
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6 \usepackage{subfigure}
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7
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8 \begin{document}
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9 \title{Generating and Exploiting Perturbed and Multi-Task Handwritten Training Data for Deep Architectures}
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10 \author{The IFT6266 Gang}
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11 \date{April 2010, Technical Report, Dept. IRO, U. Montreal}
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12
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13 \maketitle
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14
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15 \begin{abstract}
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16 Recent theoretical and empirical work in statistical machine learning has
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17 demonstrated the importance of learning algorithms for deep
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18 architectures, i.e., function classes obtained by composing multiple
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19 non-linear transformations. In the area of handwriting recognition,
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20 deep learning algorithms
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21 had been evaluated on rather small datasets with a few tens of thousands
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22 of examples. Here we propose a powerful generator of variations
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23 of examples for character images based on a pipeline of stochastic
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24 transformations that include not only the usual affine transformations
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25 but also the addition of slant, local elastic deformations, changes
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26 in thickness, background images, grey level, contrast, occlusion, and
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27 various types of pixel and spatially correlated noise.
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28 We evaluate a deep learning algorithm (Stacked Denoising Autoencoders)
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29 on the task of learning to classify digits and letters transformed
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30 with this pipeline, using the hundreds of millions of generated examples
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31 and testing on the full 62-class NIST test set.
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32 We find that the SDA outperforms its
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33 shallow counterpart, an ordinary Multi-Layer Perceptron,
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34 and that it is better able to take advantage of the additional
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35 generated data, as well as better able to take advantage of
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36 the multi-task setting, i.e.,
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37 training from more classes than those of interest in the end.
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38 In fact, we find that the SDA reaches human performance as
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39 estimated by the Amazon Mechanical Turk on the 62-class NIST test characters.
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40 \end{abstract}
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41
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42 \section{Introduction}
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43
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44 Deep Learning has emerged as a promising new area of research in
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45 statistical machine learning (see~\emcite{Bengio-2009} for a review).
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46 Learning algorithms for deep architectures are centered on the learning
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47 of useful representations of data, which are better suited to the task at hand.
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48 This is in great part inspired by observations of the mammalian visual cortex,
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49 which consists of a chain of processing elements, each of which is associated with a
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50 different representation. In fact,
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51 it was found recently that the features learnt in deep architectures resemble
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52 those observed in the first two of these stages (in areas V1 and V2
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53 of visual cortex)~\cite{HonglakL2008}.
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54 Processing images typically involves transforming the raw pixel data into
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55 new {\bf representations} that can be used for analysis or classification.
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56 For example, a principal component analysis representation linearly projects
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57 the input image into a lower-dimensional feature space.
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58 Why learn a representation? Current practice in the computer vision
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59 literature converts the raw pixels into a hand-crafted representation
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60 (e.g.\ SIFT features~\cite{Lowe04}), but deep learning algorithms
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61 tend to discover similar features in their first few
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62 levels~\cite{HonglakL2008,ranzato-08,Koray-08,VincentPLarochelleH2008-very-small}.
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63 Learning increases the
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64 ease and practicality of developing representations that are at once
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65 tailored to specific tasks, yet are able to borrow statistical strength
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66 from other related tasks (e.g., modeling different kinds of objects). Finally, learning the
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67 feature representation can lead to higher-level (more abstract, more
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68 general) features that are more robust to unanticipated sources of
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69 variance extant in real data.
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70
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71 Whereas a deep architecture can in principle be more powerful than a
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72 shallow one in terms of representation, depth appears to render the
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73 training problem more difficult in terms of optimization and local minima.
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74 It is also only recently that successful algorithms were proposed to
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75 overcome some of these difficulties. All are based on unsupervised
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76 learning, often in an greedy layer-wise ``unsupervised pre-training''
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77 stage~\cite{Bengio-2009}. One of these layer initialization techniques,
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78 applied here, is the Denoising
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79 Auto-Encoder~(DEA)~\cite{VincentPLarochelleH2008-very-small}, which
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80 performed similarly or better than previously proposed Restricted Boltzmann
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81 Machines in terms of unsupervised extraction of a hierarchy of features
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82 useful for classification. The principle is that each layer starting from
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83 the bottom is trained to encode their input (the output of the previous
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84 layer) and try to reconstruct it from a corrupted version of it. After this
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85 unsupervised initialization, the stack of denoising auto-encoders can be
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86 converted into a deep supervised feedforward neural network and trained by
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87 stochastic gradient descent.
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88
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89
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90 \section{Perturbation and Transformation of Character Images}
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91
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92 This section describes the different transformations we used to generate data, in their order.
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93 The code for these transformations (mostly python) is available at
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94 {\tt http://anonymous.url.net}. All the modules in the pipeline share
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95 a global control parameter ($0 \le complexity \le 1$) that allows one to modulate the
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96 amount of deformation or noise introduced.
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97
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98 We can differentiate two important parts in the pipeline. The first one,
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99 from slant to pinch, performs transformations of the character. The second
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100 part, from blur to contrast, adds noise to the image.
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101
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102 \subsection{Slant}
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103
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104 We mimic slant by shifting each row of the image
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105 proportionally to its height: $shift = round(slant \times height)$.
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106 The $slant$ coefficient can be negative or positive with equal probability
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107 and its value is randomly sampled according to the complexity level:
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108 $slant \sim U[0,complexity]$, so the
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109 maximum displacement for the lowest or highest pixel line is of
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110 $round(complexity \times 32)$.
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111
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112 ---
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113
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114 In order to mimic a slant effect, we simply shift each row of the image
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115 proportionnaly to its height: $shift = round(slant \times height)$. We
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116 round the shift in order to have a discret displacement. We do not use a
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117 filter to smooth the result in order to save computing time and also
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118 because latter transformations have similar effects.
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119
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120 The $slant$ coefficient can be negative or positive with equal probability
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121 and its value is randomly sampled according to the complexity level. In
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122 our case we take uniformly a number in the range $[0,complexity]$, so the
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123 maximum displacement for the lowest or highest pixel line is of
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124 $round(complexity \times 32)$.
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125
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126
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127 \subsection{Thickness}
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128
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129 Morphological operators of dilation and erosion~\citep{Haralick87,Serra82}
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130 are applied. The neighborhood of each pixel is multiplied
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131 element-wise with a {\em structuring element} matrix.
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132 The pixel value is replaced by the maximum or the minimum of the resulting
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133 matrix, respectively for dilation or erosion. Ten different structural elements with
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134 increasing dimensions (largest is $5\times5$) were used. For each image,
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135 randomly sample the operator type (dilation or erosion) with equal probability and one structural
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136 element from a subset of the $n$ smallest structuring elements where $n$ is
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137 $round(10 \times complexity)$ for dilation and $round(6 \times complexity)$
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138 for erosion. A neutral element is always present in the set, and if it is
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139 chosen no transformation is applied. Erosion allows only the six
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140 smallest structural elements because when the character is too thin it may
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141 be completely erased.
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142
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143 ---
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144
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145 To change the thickness of the characters we used morpholigical operators:
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146 dilation and erosion~\cite{Haralick87,Serra82}.
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147
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148 The basic idea of such transform is, for each pixel, to multiply in the
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149 element-wise manner its neighbourhood with a matrix called the structuring
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150 element. Then for dilation we remplace the pixel value by the maximum of
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151 the result, or the minimum for erosion. This will dilate or erode objects
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152 in the image and the strength of the transform only depends on the
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153 structuring element.
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154
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155 We used ten different structural elements with increasing dimensions (the
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156 biggest is $5\times5$). for each image, we radomly sample the operator
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157 type (dilation or erosion) with equal probability and one structural
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158 element from a subset of the $n$ smallest structuring elements where $n$ is
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159 $round(10 \times complexity)$ for dilation and $round(6 \times complexity)$
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160 for erosion. A neutral element is always present in the set, if it is
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161 chosen the transformation is not applied. Erosion allows only the six
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162 smallest structural elements because when the character is too thin it may
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163 erase it completly.
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164
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165 \subsection{Affine Transformations}
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166
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167 A $2 \times 3$ affine transform matrix (with
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168 6 parameters $(a,b,c,d,e,f)$) is sampled according to the $complexity$ level.
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169 Each pixel $(x,y)$ of the output image takes the value of the pixel
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170 nearest to $(ax+by+c,dx+ey+f)$ in the input image. This
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171 produces scaling, translation, rotation and shearing.
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172 The marginal distributions of $(a,b,c,d,e,f)$ have been tuned by hand to
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173 forbid important rotations (not to confuse classes) but to give good
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174 variability of the transformation: $a$ and $d$ $\sim U[1-3 \times
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175 complexity,1+3 \times complexity]$, $b$ and $e$ $\sim[-3 \times complexity,3
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176 \times complexity]$ and $c$ and $f$ $\sim U[-4 \times complexity, 4 \times
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177 complexity]$.
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178
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179 ----
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180
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181 We generate an affine transform matrix according to the complexity level,
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182 then we apply it directly to the image. The matrix is of size $2 \times
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183 3$, so we can represent it by six parameters $(a,b,c,d,e,f)$. Formally,
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184 for each pixel $(x,y)$ of the output image, we give the value of the pixel
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185 nearest to : $(ax+by+c,dx+ey+f)$, in the input image. This allows to
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186 produce scaling, translation, rotation and shearing variances.
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187
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188 The sampling of the parameters $(a,b,c,d,e,f)$ have been tuned by hand to
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189 forbid important rotations (not to confuse classes) but to give good
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190 variability of the transformation. For each image we sample uniformly the
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191 parameters in the following ranges: $a$ and $d$ in $[1-3 \times
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192 complexity,1+3 \times complexity]$, $b$ and $e$ in $[-3 \times complexity,3
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193 \times complexity]$ and $c$ and $f$ in $[-4 \times complexity, 4 \times
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194 complexity]$.
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195
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196
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197 \subsection{Local Elastic Deformations}
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198
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199 This filter induces a ``wiggly'' effect in the image, following~\citet{SimardSP03-short},
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200 which provides more details.
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201 Two ``displacements'' fields are generated and applied, for horizontal
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202 and vertical displacements of pixels.
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203 To generate a pixel in either field, first a value between -1 and 1 is
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204 chosen from a uniform distribution. Then all the pixels, in both fields, are
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205 multiplied by a constant $\alpha$ which controls the intensity of the
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206 displacements (larger $\alpha$ translates into larger wiggles).
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207 Each field is convolved with a Gaussian 2D kernel of
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208 standard deviation $\sigma$. Visually, this results in a blur.
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209 $\alpha = \sqrt[3]{complexity} \times 10.0$ and $\sigma = 10 - 7 \times
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210 \sqrt[3]{complexity}$.
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211
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212 ----
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213
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214 This filter induces a "wiggly" effect in the image. The description here
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215 will be brief, as the algorithm follows precisely what is described in
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216 \cite{SimardSP03}.
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217
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218 The general idea is to generate two "displacements" fields, for horizontal
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219 and vertical displacements of pixels. Each of these fields has the same
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220 size as the original image.
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221
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222 When generating the transformed image, we'll loop over the x and y
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223 positions in the fields and select, as a value, the value of the pixel in
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224 the original image at the (relative) position given by the displacement
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225 fields for this x and y. If the position we'd retrieve is outside the
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226 borders of the image, we use a 0 value instead.
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227
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228 To generate a pixel in either field, first a value between -1 and 1 is
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229 chosen from a uniform distribution. Then all the pixels, in both fields, is
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230 multiplied by a constant $\alpha$ which controls the intensity of the
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231 displacements (bigger $\alpha$ translates into larger wiggles).
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232
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233 As a final step, each field is convoluted with a Gaussian 2D kernel of
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234 standard deviation $\sigma$. Visually, this results in a "blur"
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235 filter. This has the effect of making values next to each other in the
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236 displacement fields similar. In effect, this makes the wiggles more
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237 coherent, less noisy.
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238
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239 As displacement fields were long to compute, 50 pairs of fields were
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240 generated per complexity in increments of 0.1 (50 pairs for 0.1, 50 pairs
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241 for 0.2, etc.), and afterwards, given a complexity, we selected randomly
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242 among the 50 corresponding pairs.
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243
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244 $\sigma$ and $\alpha$ were linked to complexity through the formulas
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245 $\alpha = \sqrt[3]{complexity} \times 10.0$ and $\sigma = 10 - 7 \times
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246 \sqrt[3]{complexity}$.
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247
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248
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249 \subsection{Pinch}
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250
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251 This is a GIMP filter called ``Whirl and
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252 pinch'', but whirl was set to 0. A pinch is ``similar to projecting the image onto an elastic
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253 surface and pressing or pulling on the center of the surface'' (GIMP documentation manual).
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254 For a square input image, this is akin to drawing a circle of
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255 radius $r$ around a center point $C$. Any point (pixel) $P$ belonging to
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256 that disk (region inside circle) will have its value recalculated by taking
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257 the value of another ``source'' pixel in the original image. The position of
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258 that source pixel is found on the line that goes through $C$ and $P$, but
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259 at some other distance $d_2$. Define $d_1$ to be the distance between $P$
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260 and $C$. $d_2$ is given by $d_2 = sin(\frac{\pi{}d_1}{2r})^{-pinch} \times
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261 d_1$, where $pinch$ is a parameter to the filter.
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262 The actual value is given by bilinear interpolation considering the pixels
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263 around the (non-integer) source position thus found.
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264 Here $pinch \sim U[-complexity, 0.7 \times complexity]$.
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265
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266 ---
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267
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268 This is another GIMP filter we used. The filter is in fact named "Whirl and
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269 pinch", but we don't use the "whirl" part (whirl is set to 0). As described
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270 in GIMP, a pinch is "similar to projecting the image onto an elastic
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271 surface and pressing or pulling on the center of the surface".
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272
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273 Mathematically, for a square input image, think of drawing a circle of
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274 radius $r$ around a center point $C$. Any point (pixel) $P$ belonging to
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275 that disk (region inside circle) will have its value recalculated by taking
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276 the value of another "source" pixel in the original image. The position of
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277 that source pixel is found on the line thats goes through $C$ and $P$, but
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278 at some other distance $d_2$. Define $d_1$ to be the distance between $P$
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279 and $C$. $d_2$ is given by $d_2 = sin(\frac{\pi{}d_1}{2r})^{-pinch} \times
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280 d_1$, where $pinch$ is a parameter to the filter.
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281
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282 If the region considered is not square then, before computing $d_2$, the
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283 smallest dimension (x or y) is stretched such that we may consider the
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284 region as if it was square. Then, after $d_2$ has been computed and
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285 corresponding components $d_2\_x$ and $d_2\_y$ have been found, the
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286 component corresponding to the stretched dimension is compressed back by an
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287 inverse ratio.
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288
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289 The actual value is given by bilinear interpolation considering the pixels
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290 around the (non-integer) source position thus found.
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291
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292 The value for $pinch$ in our case was given by sampling from an uniform
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293 distribution over the range $[-complexity, 0.7 \times complexity]$.
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294
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295 \subsection{Motion Blur}
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296
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297 This is a ``linear motion blur'' in GIMP
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298 terminology, with two parameters, $length$ and $angle$. The value of
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299 a pixel in the final image is approximately the mean value of the $length$ first pixels
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300 found by moving in the $angle$ direction.
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301 Here $angle \sim U[0,360]$ degrees, and $length \sim {\rm Normal}(0,(3 \times complexity)^2)$.
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302
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303 ----
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304
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305 This is a GIMP filter we applied, a "linear motion blur" in GIMP
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306 terminology. The description will be brief as it is a well-known filter.
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307
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308 This algorithm has two input parameters, $length$ and $angle$. The value of
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309 a pixel in the final image is the mean value of the $length$ first pixels
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310 found by moving in the $angle$ direction. An approximation of this idea is
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311 used, as we won't fall onto precise pixels by following that
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312 direction. This is done using the Bresenham line algorithm.
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313
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314 The angle, in our case, is chosen from a uniform distribution over
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315 $[0,360]$ degrees. The length, though, depends on the complexity; it's
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316 sampled from a Gaussian distribution of mean 0 and standard deviation
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317 $\sigma = 3 \times complexity$.
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318
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319 \subsection{Occlusion}
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320
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321 Selects a random rectangle from an {\em occluder} character
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322 images and places it over the original {\em occluded} character
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323 image. Pixels are combined by taking the max(occluder,occluded),
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324 closer to black. The rectangle corners
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325 are sampled so that larger complexity gives larger rectangles.
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326 The destination position in the occluded image are also sampled
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327 according to a normal distribution (see more details in~\citet{ift6266-tr-anonymous}).
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328 This filter has a probability of 60\% of not being applied.
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329
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330 ---
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331
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332 This filter selects random parts of other (hereafter "occlusive") letter
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333 images and places them over the original letter (hereafter "occluded")
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334 image. To be more precise, having selected a subregion of the occlusive
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335 image and a desination position in the occluded image, to determine the
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336 final value for a given overlapping pixel, it selects whichever pixel is
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337 the lightest. As a reminder, the background value is 0, black, so the value
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338 nearest to 1 is selected.
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339
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340 To select a subpart of the occlusive image, four numbers are generated. For
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341 compability with the code, we'll call them "haut", "bas", "gauche" and
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342 "droite" (respectively meaning top, bottom, left and right). Each of these
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343 numbers is selected according to a Gaussian distribution of mean $8 \times
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344 complexity$ and standard deviation $2$. This means the largest the
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345 complexity is, the biggest the occlusion will be. The absolute value is
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346 taken, as the numbers must be positive, and the maximum value is capped at
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347 15.
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348
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349 These four sizes collectively define a window centered on the middle pixel
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350 of the occlusive image. This is the part that will be extracted as the
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351 occlusion.
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352
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353 The next step is to select a destination position in the occluded
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354 image. Vertical and horizontal displacements $y\_arrivee$ and $x\_arrivee$
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parents: 461
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355 are selected according to Gaussian distributions of mean 0 and of standard
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356 deviations of, respectively, 3 and 2. Then an horizontal placement mode,
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357 $place$, is selected to be of three values meaning
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358 left, middle or right.
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359
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360 If $place$ is "middle", the occlusion will be horizontally centered
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361 around the horizontal middle of the occluded image, then shifted according
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362 to $x\_arrivee$. If $place$ is "left", it will be placed on the left of
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363 the occluded image, then displaced right according to $x\_arrivee$. The
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364 contrary happens if $place$ is $right$.
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365
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366 In both the horizontal and vertical positionning, the maximum position in
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367 either direction is such that the selected occlusion won't go beyond the
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368 borders of the occluded image.
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369
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370 This filter has a probability of not being applied, at all, of 60\%.
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371
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372
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373 \subsection{Pixel Permutation}
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374
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375 This filter permutes neighbouring pixels. It selects first
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376 $\frac{complexity}{3}$ pixels randomly in the image. Each of them are then
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377 sequentially exchanged with one other pixel in its $V4$ neighbourhood. The number
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378 of exchanges to the left, right, top, bottom is equal or does not differ
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379 from more than 1 if the number of selected pixels is not a multiple of 4.
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380 % TODO: The previous sentence is hard to parse
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381 This filter has a probability of 80\% of not being applied.
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382
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383 ---
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384
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385 This filter permuts neighbouring pixels. It selects first
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386 $\frac{complexity}{3}$ pixels randomly in the image. Each of them are then
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387 sequentially exchanged to one other pixel in its $V4$ neighbourhood. Number
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388 of exchanges to the left, right, top, bottom are equal or does not differ
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389 from more than 1 if the number of selected pixels is not a multiple of 4.
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parents: 431
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390
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391 It has has a probability of not being applied, at all, of 80\%.
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392
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393
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394 \subsection{Gaussian Noise}
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395
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396 This filter simply adds, to each pixel of the image independently, a
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parents: 479
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397 noise $\sim Normal(0(\frac{complexity}{10})^2)$.
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398 It has a probability of 70\% of not being applied.
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399
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400 ---
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401
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402 This filter simply adds, to each pixel of the image independently, a
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403 Gaussian noise of mean $0$ and standard deviation $\frac{complexity}{10}$.
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parents: 425
diff changeset
404
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parents: 425
diff changeset
405 It has has a probability of not being applied, at all, of 70\%.
a7fab59de174 change order of transformations
Xavier Glorot <glorotxa@iro.umontreal.ca>
parents: 425
diff changeset
406
a7fab59de174 change order of transformations
Xavier Glorot <glorotxa@iro.umontreal.ca>
parents: 425
diff changeset
407
379
a21a174c1c18 added writeup skeleton
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
408 \subsection{Background Images}
415
1e9788ce1680 Added the parts concerning the transformations I'd announced I'd do: Local elastic deformations; occlusions; gimp transformations; salt and pepper noise; background images
fsavard
parents: 411
diff changeset
409
541
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
410 Following~\citet{Larochelle-jmlr-2009}, this transformation adds a random
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
411 background behind the letter. The background is chosen by first selecting,
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
412 at random, an image from a set of images. Then a 32$\times$32 sub-region
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
413 of that image is chosen as the background image (by sampling position
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
414 uniformly while making sure not to cross image borders).
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
415 To combine the original letter image and the background image, contrast
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
416 adjustments are made. We first get the maximal values (i.e. maximal
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
417 intensity) for both the original image and the background image, $maximage$
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
418 and $maxbg$. We also have a parameter $contrast \sim U[complexity, 1]$.
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
419 Each background pixel value is multiplied by $\frac{max(maximage -
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
420 contrast, 0)}{maxbg}$ (higher contrast yield darker
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
421 background). The output image pixels are max(background,original).
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
422
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
423 ---
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
424
462
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
425 Following~\cite{Larochelle-jmlr-2009}, this transformation adds a random
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
426 background behind the letter. The background is chosen by first selecting,
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
427 at random, an image from a set of images. Then we choose a 32x32 subregion
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
428 of that image as the background image (by sampling x and y positions
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
429 uniformly while making sure not to cross image borders).
415
1e9788ce1680 Added the parts concerning the transformations I'd announced I'd do: Local elastic deformations; occlusions; gimp transformations; salt and pepper noise; background images
fsavard
parents: 411
diff changeset
430
462
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
431 To combine the original letter image and the background image, contrast
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
432 adjustments are made. We first get the maximal values (i.e. maximal
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
433 intensity) for both the original image and the background image, $maximage$
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
434 and $maxbg$. We also have a parameter, $contrast$, given by sampling from a
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
435 uniform distribution over $[complexity, 1]$.
415
1e9788ce1680 Added the parts concerning the transformations I'd announced I'd do: Local elastic deformations; occlusions; gimp transformations; salt and pepper noise; background images
fsavard
parents: 411
diff changeset
436
462
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
437 Once we have all these numbers, we first adjust the values for the
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
438 background image. Each pixel value is multiplied by $\frac{max(maximage -
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
439 contrast, 0)}{maxbg}$. Therefore the higher the contrast, the darkest the
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
440 background will be.
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
441
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
442 The final image is found by taking the brightest (i.e. value nearest to 1)
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
443 pixel from either the background image or the corresponding pixel in the
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
444 original image.
415
1e9788ce1680 Added the parts concerning the transformations I'd announced I'd do: Local elastic deformations; occlusions; gimp transformations; salt and pepper noise; background images
fsavard
parents: 411
diff changeset
445
379
a21a174c1c18 added writeup skeleton
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
446 \subsection{Salt and Pepper Noise}
415
1e9788ce1680 Added the parts concerning the transformations I'd announced I'd do: Local elastic deformations; occlusions; gimp transformations; salt and pepper noise; background images
fsavard
parents: 411
diff changeset
447
541
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
448 This filter adds noise $\sim U[0,1]$ to random subsets of pixels.
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
449 The number of selected pixels is $0.2 \times complexity$.
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
450 This filter has a probability of not being applied at all of 75\%.
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
451
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
452 ---
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
453
462
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
454 This filter adds noise to the image by randomly selecting a certain number
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
455 of them and, for those selected pixels, assign a random value according to
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
456 a uniform distribution over the $[0,1]$ ranges. This last distribution does
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
457 not change according to complexity. Instead, the number of selected pixels
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
458 does: the proportion of changed pixels corresponds to $complexity / 5$,
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
459 which means, as a maximum, 20\% of the pixels will be randomized. On the
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
460 lowest extreme, no pixel is changed.
415
1e9788ce1680 Added the parts concerning the transformations I'd announced I'd do: Local elastic deformations; occlusions; gimp transformations; salt and pepper noise; background images
fsavard
parents: 411
diff changeset
461
420
a3a4a9c6476d added transformations description and began dataset descriptions
Xavier Glorot <glorotxa@iro.umontreal.ca>
parents: 417
diff changeset
462 This filter also has a probability of not being applied, at all, of 75\%.
415
1e9788ce1680 Added the parts concerning the transformations I'd announced I'd do: Local elastic deformations; occlusions; gimp transformations; salt and pepper noise; background images
fsavard
parents: 411
diff changeset
463
379
a21a174c1c18 added writeup skeleton
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
464 \subsection{Spatially Gaussian Noise}
426
a7fab59de174 change order of transformations
Xavier Glorot <glorotxa@iro.umontreal.ca>
parents: 425
diff changeset
465
541
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
466 Different regions of the image are spatially smoothed.
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
467 The image is convolved with a symmetric Gaussian kernel of
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
468 size and variance chosen uniformly in the ranges $[12,12 + 20 \times
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
469 complexity]$ and $[2,2 + 6 \times complexity]$. The result is normalized
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
470 between $0$ and $1$. We also create a symmetric averaging window, of the
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
471 kernel size, with maximum value at the center. For each image we sample
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
472 uniformly from $3$ to $3 + 10 \times complexity$ pixels that will be
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
473 averaging centers between the original image and the filtered one. We
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
474 initialize to zero a mask matrix of the image size. For each selected pixel
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
475 we add to the mask the averaging window centered to it. The final image is
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
476 computed from the following element-wise operation: $\frac{image + filtered
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
477 image \times mask}{mask+1}$.
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
478 This filter has a probability of not being applied at all of 75\%.
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
479
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
480 ----
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
481
462
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
482 The aim of this transformation is to filter, with a gaussian kernel,
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
483 different regions of the image. In order to save computing time we decided
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
484 to convolve the whole image only once with a symmetric gaussian kernel of
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
485 size and variance choosen uniformly in the ranges: $[12,12 + 20 \times
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
486 complexity]$ and $[2,2 + 6 \times complexity]$. The result is normalized
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
487 between $0$ and $1$. We also create a symmetric averaging window, of the
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
488 kernel size, with maximum value at the center. For each image we sample
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
489 uniformly from $3$ to $3 + 10 \times complexity$ pixels that will be
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
490 averaging centers between the original image and the filtered one. We
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
491 initialize to zero a mask matrix of the image size. For each selected pixel
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
492 we add to the mask the averaging window centered to it. The final image is
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
493 computed from the following element-wise operation: $\frac{image + filtered
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
494 image \times mask}{mask+1}$.
420
a3a4a9c6476d added transformations description and began dataset descriptions
Xavier Glorot <glorotxa@iro.umontreal.ca>
parents: 417
diff changeset
495
a3a4a9c6476d added transformations description and began dataset descriptions
Xavier Glorot <glorotxa@iro.umontreal.ca>
parents: 417
diff changeset
496 This filter has a probability of not being applied, at all, of 75\%.
a3a4a9c6476d added transformations description and began dataset descriptions
Xavier Glorot <glorotxa@iro.umontreal.ca>
parents: 417
diff changeset
497
462
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
498 \subsection{Scratches}
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
499
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
500 The scratches module places line-like white patches on the image. The
541
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
501 lines are heavily transformed images of the digit ``1'' (one), chosen
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
502 at random among five thousands such 1 images. The 1 image is
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
503 randomly cropped and rotated by an angle $\sim Normal(0,(100 \times
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
504 complexity)^2$, using bi-cubic interpolation,
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
505 Two passes of a grey-scale morphological erosion filter
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
506 are applied, reducing the width of the line
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
507 by an amount controlled by $complexity$.
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
508 This filter is only applied only 15\% of the time. When it is applied, 50\%
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
509 of the time, only one patch image is generated and applied. In 30\% of
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
510 cases, two patches are generated, and otherwise three patches are
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
511 generated. The patch is applied by taking the maximal value on any given
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
512 patch or the original image, for each of the 32x32 pixel locations.
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
513
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
514 ---
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
515
8aad1c6ec39a reduction espace
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 479
diff changeset
516 The scratches module places line-like white patches on the image. The
462
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
517 lines are in fact heavily transformed images of the digit "1" (one), chosen
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
518 at random among five thousands such start images of this digit.
428
9fcd0215b8d5 Added text for ratures filter
fsavard
parents: 427
diff changeset
519
462
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
520 Once the image is selected, the transformation begins by finding the first
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
521 $top$, $bottom$, $right$ and $left$ non-zero pixels in the image. It is
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
522 then cropped to the region thus delimited, then this cropped version is
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
523 expanded to $32\times32$ again. It is then rotated by a random angle having a
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
524 Gaussian distribution of mean 90 and standard deviation $100 \times
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
525 complexity$ (in degrees). The rotation is done with bicubic interpolation.
428
9fcd0215b8d5 Added text for ratures filter
fsavard
parents: 427
diff changeset
526
462
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
527 The rotated image is then resized to $50\times50$, with anti-aliasing. In
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
528 that image, we crop the image again by selecting a region delimited
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
529 horizontally to $left$ to $left+32$ and vertically by $top$ to $top+32$.
428
9fcd0215b8d5 Added text for ratures filter
fsavard
parents: 427
diff changeset
530
462
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
531 Once this is done, two passes of a greyscale morphological erosion filter
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
532 are applied. Put briefly, this erosion filter reduces the width of the line
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
533 by a certain $smoothing$ amount. For small complexities (< 0.5),
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
534 $smoothing$ is 6, so the line is very small. For complexities ranging from
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
535 0.25 to 0.5, $smoothing$ is 5. It is 4 for complexities 0.5 to 0.75, and 3
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
536 for higher complexities.
428
9fcd0215b8d5 Added text for ratures filter
fsavard
parents: 427
diff changeset
537
462
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
538 To compensate for border effects, the image is then cropped to 28x28 by
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
539 removing two pixels everywhere on the borders, then expanded to 32x32
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
540 again. The pixel values are then linearly expanded such that the minimum
f59af1648d83 cleaner le techreport
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
541 value is 0 and the maximal one is 1. Then, 50\% of the time, the image is
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parents: 461
diff changeset
542 vertically flipped.
428
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parents: 427
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543
462
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parents: 461
diff changeset
544 This filter is only applied only 15\% of the time. When it is applied, 50\%
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parents: 461
diff changeset
545 of the time, only one patch image is generated and applied. In 30\% of
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parents: 461
diff changeset
546 cases, two patches are generated, and otherwise three patches are
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parents: 461
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547 generated. The patch is applied by taking the maximal value on any given
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parents: 461
diff changeset
548 patch or the original image, for each of the 32x32 pixel locations.
420
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parents: 417
diff changeset
549
541
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parents: 479
diff changeset
550 \subsection{Grey Level and Contrast Changes}
426
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Xavier Glorot <glorotxa@iro.umontreal.ca>
parents: 425
diff changeset
551
541
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parents: 479
diff changeset
552 This filter changes the contrast and may invert the image polarity (white
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parents: 479
diff changeset
553 on black to black on white). The contrast $C$ is defined here as the
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parents: 479
diff changeset
554 difference between the maximum and the minimum pixel value of the image.
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parents: 479
diff changeset
555 Contrast $\sim U[1-0.85 \times complexity,1]$ (so contrast $\geq 0.15$).
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parents: 479
diff changeset
556 The image is normalized into $[\frac{1-C}{2},1-\frac{1-C}{2}]$. The
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parents: 479
diff changeset
557 polarity is inverted with $0.5$ probability.
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parents: 479
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558
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parents: 479
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559 ---
462
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parents: 461
diff changeset
560 This filter changes the constrast and may invert the image polarity (white
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
561 on black to black on white). The contrast $C$ is defined here as the
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 461
diff changeset
562 difference between the maximum and the minimum pixel value of the image. A
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parents: 461
diff changeset
563 contrast value is sampled uniformly between $1$ and $1-0.85 \times
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parents: 461
diff changeset
564 complexity$ (this insure a minimum constrast of $0.15$). We then simply
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parents: 461
diff changeset
565 normalize the image to the range $[\frac{1-C}{2},1-\frac{1-C}{2}]$. The
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parents: 461
diff changeset
566 polarity is inverted with $0.5$ probability.
420
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parents: 417
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567
379
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parents:
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568
393
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diff changeset
569 \begin{figure}[h]
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parents: 392
diff changeset
570 \resizebox{.99\textwidth}{!}{\includegraphics{images/example_t.png}}\\
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parents: 392
diff changeset
571 \caption{Illustration of the pipeline of stochastic
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parents: 392
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572 transformations applied to the image of a lower-case t
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parents: 392
diff changeset
573 (the upper left image). Each image in the pipeline (going from
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parents: 392
diff changeset
574 left to right, first top line, then bottom line) shows the result
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parents: 392
diff changeset
575 of applying one of the modules in the pipeline. The last image
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parents: 392
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576 (bottom right) is used as training example.}
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parents: 392
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577 \label{fig:pipeline}
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578 \end{figure}
379
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579
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parents: 417
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580
479
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parents: 477
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581 \begin{figure}[h]
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parents: 477
diff changeset
582 \resizebox{.99\textwidth}{!}{\includegraphics{images/transfo.png}}\\
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parents: 477
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583 \caption{Illustration of each transformation applied to the same image
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parents: 477
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584 of the upper-case h (upper-left image). first row (from left to rigth) : original image, slant,
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parents: 477
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585 thickness, affine transformation, local elastic deformation; second row (from left to rigth) :
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parents: 477
diff changeset
586 pinch, motion blur, occlusion, pixel permutation, gaussian noise; third row (from left to rigth) :
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parents: 477
diff changeset
587 background image, salt and pepper noise, spatially gaussian noise, scratches,
541
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parents: 479
diff changeset
588 grey level and contrast changes.}
479
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589 \label{fig:transfo}
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590 \end{figure}
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591
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592
379
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593 \section{Experimental Setup}
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parents:
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594
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parents:
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595 \subsection{Training Datasets}
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parents:
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596
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597 \subsubsection{Data Sources}
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598
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parents:
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599 \begin{itemize}
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parents:
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600 \item {\bf NIST}
434
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601 The NIST Special Database 19 (NIST19) is a very widely used dataset for training and testing OCR systems.
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goldfinger
parents: 432
diff changeset
602 The dataset is composed with over 800 000 digits and characters (upper and lower cases), with hand checked classifications,
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goldfinger
parents: 432
diff changeset
603 extracted from handwritten sample forms of 3600 writers. The characters are labelled by one of the 62 classes
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goldfinger
parents: 432
diff changeset
604 corresponding to "0"-"9","A"-"Z" and "a"-"z". The dataset contains 8 series of different complexity.
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goldfinger
parents: 432
diff changeset
605 The fourth series, $hsf_4$, experimentally recognized to be the most difficult one for classification task is recommended
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goldfinger
parents: 432
diff changeset
606 by NIST as testing set and is used in our work for that purpose.
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diff changeset
607 The performances reported by previous work on that dataset mostly use only the digits.
432
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diff changeset
608 Here we use the whole classes both in the training and testing phase.
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609
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610
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611 \item {\bf Fonts}
477
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parents: 463
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612 In order to have a good variety of sources we downloaded an important number of free fonts from: {\tt http://anonymous.url.net}
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diff changeset
613 %real adress {\tt http://cg.scs.carleton.ca/~luc/freefonts.html}
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parents: 463
diff changeset
614 in addition to Windows 7's, this adds up to a total of $9817$ different fonts that we can choose uniformly.
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parents: 463
diff changeset
615 The ttf file is either used as input of the Captcha generator (see next item) or, by producing a corresponding image,
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616 directly as input to our models.
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parents: 463
diff changeset
617 %Guillaume are there other details I forgot on the font selection?
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618
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619 \item {\bf Captchas}
432
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620 The Captcha data source is an adaptation of the \emph{pycaptcha} library (a python based captcha generator library) for
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goldfinger
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diff changeset
621 generating characters of the same format as the NIST dataset. The core of this data source is composed with a random character
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622 generator and various kinds of tranformations similar to those described in the previous sections.
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diff changeset
623 In order to increase the variability of the data generated, different fonts are used for generating the characters.
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624 Transformations (slant, distorsions, rotation, translation) are applied to each randomly generated character with a complexity
e2fd928a7de0 added description of nist19 and captcha data sources
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625 depending on the value of the complexity parameter provided by the user of the data source. Two levels of complexity are
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626 allowed and can be controlled via an easy to use facade class.
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627 \item {\bf OCR data}
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628 \end{itemize}
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629
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parents:
diff changeset
630 \subsubsection{Data Sets}
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parents:
diff changeset
631 \begin{itemize}
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parents:
diff changeset
632 \item {\bf P07}
420
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diff changeset
633 The dataset P07 is sampled with our transformation pipeline with a complexity parameter of $0.7$.
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634 For each new exemple to generate, we choose one source with the following probability: $0.1$ for the fonts,
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635 $0.25$ for the captchas, $0.25$ for OCR data and $0.4$ for NIST. We apply all the transformations in their order
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diff changeset
636 and for each of them we sample uniformly a complexity in the range $[0,0.7]$.
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637 \item {\bf NISTP} {\em ne pas utiliser PNIST mais NISTP, pour rester politically correct...}
463
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diff changeset
638 NISTP is equivalent to P07 (complexity parameter of $0.7$ with the same sources proportion) except that we only apply transformations from slant to pinch. Therefore, the character is transformed
420
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diff changeset
639 but no additionnal noise is added to the image, this gives images closer to the NIST dataset.
379
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640 \end{itemize}
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641
452
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diff changeset
642 We noticed that the distribution of the training sets and the test sets differ.
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diff changeset
643 Since our validation sets are sampled from the training set, they have approximately the same distribution, but the test set has a completely different distribution as illustrated in figure \ref {setsdata}.
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644
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diff changeset
645 \begin{figure}
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diff changeset
646 \subfigure[NIST training]{\includegraphics[width=0.5\textwidth]{images/nisttrainstats}}
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647 \subfigure[NIST validation]{\includegraphics[width=0.5\textwidth]{images/nistvalidstats}}
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diff changeset
648 \subfigure[NIST test]{\includegraphics[width=0.5\textwidth]{images/nistteststats}}
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diff changeset
649 \subfigure[NISTP validation]{\includegraphics[width=0.5\textwidth]{images/nistpvalidstats}}
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650 \caption{Proportion of each class in some of the data sets}
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diff changeset
651 \label{setsdata}
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652 \end{figure}
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653
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654 \subsection{Models and their Hyperparameters}
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diff changeset
655
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656 \subsubsection{Multi-Layer Perceptrons (MLP)}
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657
410
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658 An MLP is a family of functions that are described by stacking layers of of a function similar to
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659 $$g(x) = \tanh(b+Wx)$$
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660 The input, $x$, is a $d$-dimension vector.
6330298791fb Description brève de MLP et SdA
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diff changeset
661 The output, $g(x)$, is a $m$-dimension vector.
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diff changeset
662 The parameter $W$ is a $m\times d$ matrix and is called the weight matrix.
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663 The parameter $b$ is a $m$-vector and is called the bias vector.
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diff changeset
664 The non-linearity (here $\tanh$) is applied element-wise to the output vector.
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parents: 407
diff changeset
665 Usually the input is referred to a input layer and similarly for the output.
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diff changeset
666 You can of course chain several such functions to obtain a more complex one.
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diff changeset
667 Here is a common example
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668 $$f(x) = c + V\tanh(b+Wx)$$
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parents: 407
diff changeset
669 In this case the intermediate layer corresponding to $\tanh(b+Wx)$ is called a hidden layer.
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parents: 407
diff changeset
670 Here the output layer does not have the same non-linearity as the hidden layer.
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parents: 407
diff changeset
671 This is a common case where some specialized non-linearity is applied to the output layer only depending on the task at hand.
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parents: 407
diff changeset
672
6330298791fb Description brève de MLP et SdA
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parents: 407
diff changeset
673 If you put 3 or more hidden layers in such a network you obtain what is called a deep MLP.
411
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Arnaud Bergeron <abergeron@gmail.com>
parents: 410
diff changeset
674 The parameters to adapt are the weight matrix and the bias vector for each layer.
410
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Arnaud Bergeron <abergeron@gmail.com>
parents: 407
diff changeset
675
379
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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676 \subsubsection{Stacked Denoising Auto-Encoders (SDAE)}
422
e7790db265b1 Basic text for section 3, add a bit more detail to section 4.2.2
Arnaud Bergeron <abergeron@gmail.com>
parents: 417
diff changeset
677 \label{SdA}
379
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678
410
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679 Auto-encoders are essentially a way to initialize the weights of the network to enable better generalization.
422
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Arnaud Bergeron <abergeron@gmail.com>
parents: 417
diff changeset
680 This is essentially unsupervised training where the layer is made to reconstruct its input through and encoding and decoding phase.
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Arnaud Bergeron <abergeron@gmail.com>
parents: 417
diff changeset
681 Denoising auto-encoders are a variant where the input is corrupted with random noise but the target is the uncorrupted input.
410
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Arnaud Bergeron <abergeron@gmail.com>
parents: 407
diff changeset
682 The principle behind these initialization methods is that the network will learn the inherent relation between portions of the data and be able to represent them thus helping with whatever task we want to perform.
6330298791fb Description brève de MLP et SdA
Arnaud Bergeron <abergeron@gmail.com>
parents: 407
diff changeset
683
411
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Arnaud Bergeron <abergeron@gmail.com>
parents: 410
diff changeset
684 An auto-encoder unit is formed of two MLP layers with the bottom one called the encoding layer and the top one the decoding layer.
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Arnaud Bergeron <abergeron@gmail.com>
parents: 410
diff changeset
685 Usually the top and bottom weight matrices are the transpose of each other and are fixed this way.
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Arnaud Bergeron <abergeron@gmail.com>
parents: 410
diff changeset
686 The network is trained as such and, when sufficiently trained, the MLP layer is initialized with the parameters of the encoding layer.
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Arnaud Bergeron <abergeron@gmail.com>
parents: 410
diff changeset
687 The other parameters are discarded.
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Arnaud Bergeron <abergeron@gmail.com>
parents: 410
diff changeset
688
410
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Arnaud Bergeron <abergeron@gmail.com>
parents: 407
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689 The stacked version is an adaptation to deep MLPs where you initialize each layer with a denoising auto-encoder starting from the bottom.
411
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Arnaud Bergeron <abergeron@gmail.com>
parents: 410
diff changeset
690 During the initialization, which is usually called pre-training, the bottom layer is treated as if it were an isolated auto-encoder.
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Arnaud Bergeron <abergeron@gmail.com>
parents: 410
diff changeset
691 The second and following layers receive the same treatment except that they take as input the encoded version of the data that has gone through the layers before it.
410
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Arnaud Bergeron <abergeron@gmail.com>
parents: 407
diff changeset
692 For additional details see \cite{vincent:icml08}.
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Arnaud Bergeron <abergeron@gmail.com>
parents: 407
diff changeset
693
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694 \section{Experimental Results}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
695
438
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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696 \subsection{SDA vs MLP vs Humans}
392
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 381
diff changeset
697
438
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diff changeset
698 We compare here the best MLP (according to validation set error) that we found against
a6d339033d03 added AMT
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
699 the best SDA (again according to validation set error), along with a precise estimate
a6d339033d03 added AMT
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
700 of human performance obtained via Amazon's Mechanical Turk (AMT)
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
701 service\footnote{http://mturk.com}. AMT users are paid small amounts
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
702 of money to perform tasks for which human intelligence is required.
a6d339033d03 added AMT
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
703 Mechanical Turk has been used extensively in natural language
a6d339033d03 added AMT
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
704 processing \cite{SnowEtAl2008} and vision
a6d339033d03 added AMT
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
705 \cite{SorokinAndForsyth2008,whitehill09}. AMT users where presented
a6d339033d03 added AMT
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
706 with 10 character images and asked to type 10 corresponding ascii
a6d339033d03 added AMT
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
707 characters. Hence they were forced to make a hard choice among the
a6d339033d03 added AMT
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
708 62 character classes. Three users classified each image, allowing
a6d339033d03 added AMT
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
709 to estimate inter-human variability (shown as +/- in parenthesis below).
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
710
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
711 \begin{table}
458
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 452
diff changeset
712 \caption{Overall comparison of error rates ($\pm$ std.err.) on 62 character classes (10 digits +
438
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
713 26 lower + 26 upper), except for last columns -- digits only, between deep architecture with pre-training
a6d339033d03 added AMT
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
714 (SDA=Stacked Denoising Autoencoder) and ordinary shallow architecture
458
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 452
diff changeset
715 (MLP=Multi-Layer Perceptron). The models shown are all trained using perturbed data (NISTP or P07)
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 452
diff changeset
716 and using a validation set to select hyper-parameters and other training choices.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 452
diff changeset
717 \{SDA,MLP\}0 are trained on NIST,
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 452
diff changeset
718 \{SDA,MLP\}1 are trained on NISTP, and \{SDA,MLP\}2 are trained on P07.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 452
diff changeset
719 The human error rate on digits is a lower bound because it does not count digits that were
461
9609c5cf9b6b lit. results
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 460
diff changeset
720 recognized as letters. For comparison, the results found in the literature
9609c5cf9b6b lit. results
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 460
diff changeset
721 on NIST digits classification using the same test set are included.}
438
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parents: 437
diff changeset
722 \label{tab:sda-vs-mlp-vs-humans}
392
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 381
diff changeset
723 \begin{center}
438
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 437
diff changeset
724 \begin{tabular}{|l|r|r|r|r|} \hline
458
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parents: 452
diff changeset
725 & NIST test & NISTP test & P07 test & NIST test digits \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 452
diff changeset
726 Humans& 18.2\% $\pm$.1\% & 39.4\%$\pm$.1\% & 46.9\%$\pm$.1\% & $>1.1\%$ \\ \hline
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parents: 452
diff changeset
727 SDA0 & 23.7\% $\pm$.14\% & 65.2\%$\pm$.34\% & 97.45\%$\pm$.06\% & 2.7\% $\pm$.14\%\\ \hline
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parents: 452
diff changeset
728 SDA1 & 17.1\% $\pm$.13\% & 29.7\%$\pm$.3\% & 29.7\%$\pm$.3\% & 1.4\% $\pm$.1\%\\ \hline
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parents: 452
diff changeset
729 SDA2 & 18.7\% $\pm$.13\% & 33.6\%$\pm$.3\% & 39.9\%$\pm$.17\% & 1.7\% $\pm$.1\%\\ \hline
460
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
730 MLP0 & 24.2\% $\pm$.15\% & 68.8\%$\pm$.33\% & 78.70\%$\pm$.14\% & 3.45\% $\pm$.15\% \\ \hline
458
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parents: 452
diff changeset
731 MLP1 & 23.0\% $\pm$.15\% & 41.8\%$\pm$.35\% & 90.4\%$\pm$.1\% & 3.85\% $\pm$.16\% \\ \hline
460
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
732 MLP2 & 24.3\% $\pm$.15\% & 46.0\%$\pm$.35\% & 54.7\%$\pm$.17\% & 4.85\% $\pm$.18\% \\ \hline
461
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 460
diff changeset
733 [5] & & & & 4.95\% $\pm$.18\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 460
diff changeset
734 [2] & & & & 3.71\% $\pm$.16\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 460
diff changeset
735 [3] & & & & 2.4\% $\pm$.13\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 460
diff changeset
736 [4] & & & & 2.1\% $\pm$.12\% \\ \hline
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diff changeset
737 \end{tabular}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 381
diff changeset
738 \end{center}
438
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diff changeset
739 \end{table}
379
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740
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diff changeset
741 \subsection{Perturbed Training Data More Helpful for SDAE}
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diff changeset
742
460
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743 \begin{table}
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parents: 458
diff changeset
744 \caption{Relative change in error rates due to the use of perturbed training data,
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
745 either using NISTP, for the MLP1/SDA1 models, or using P07, for the MLP2/SDA2 models.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
746 A positive value indicates that training on the perturbed data helped for the
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
747 given test set (the first 3 columns on the 62-class tasks and the last one is
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
748 on the clean 10-class digits). Clearly, the deep learning models did benefit more
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parents: 458
diff changeset
749 from perturbed training data, even when testing on clean data, whereas the MLP
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
750 trained on perturbed data performed worse on the clean digits and about the same
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
751 on the clean characters. }
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parents: 458
diff changeset
752 \label{tab:sda-vs-mlp-vs-humans}
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parents: 458
diff changeset
753 \begin{center}
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parents: 458
diff changeset
754 \begin{tabular}{|l|r|r|r|r|} \hline
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diff changeset
755 & NIST test & NISTP test & P07 test & NIST test digits \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
756 SDA0/SDA1-1 & 38\% & 84\% & 228\% & 93\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
757 SDA0/SDA2-1 & 27\% & 94\% & 144\% & 59\% \\ \hline
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parents: 458
diff changeset
758 MLP0/MLP1-1 & 5.2\% & 65\% & -13\% & -10\% \\ \hline
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parents: 458
diff changeset
759 MLP0/MLP2-1 & -0.4\% & 49\% & 44\% & -29\% \\ \hline
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parents: 458
diff changeset
760 \end{tabular}
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parents: 458
diff changeset
761 \end{center}
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parents: 458
diff changeset
762 \end{table}
458
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diff changeset
763
460
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764
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diff changeset
765 \subsection{Multi-Task Learning Effects}
379
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766
460
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767 As previously seen, the SDA is better able to benefit from the
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parents: 458
diff changeset
768 transformations applied to the data than the MLP. In this experiment we
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parents: 458
diff changeset
769 define three tasks: recognizing digits (knowing that the input is a digit),
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parents: 458
diff changeset
770 recognizing upper case characters (knowing that the input is one), and
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parents: 458
diff changeset
771 recognizing lower case characters (knowing that the input is one). We
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parents: 458
diff changeset
772 consider the digit classification task as the target task and we want to
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diff changeset
773 evaluate whether training with the other tasks can help or hurt, and
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parents: 458
diff changeset
774 whether the effect is different for MLPs versus SDAs. The goal is to find
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parents: 458
diff changeset
775 out if deep learning can benefit more (or less) from multiple related tasks
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parents: 458
diff changeset
776 (i.e. the multi-task setting) compared to a corresponding purely supervised
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parents: 458
diff changeset
777 shallow learner.
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diff changeset
778
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779 We use a single hidden layer MLP with 1000 hidden units, and a SDA
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diff changeset
780 with 3 hidden layers (1000 hidden units per layer), pre-trained and
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parents: 458
diff changeset
781 fine-tuned on NIST.
437
479f2f518fc9 added Training with More Classes than Necessary
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parents: 434
diff changeset
782
460
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783 Our results show that the MLP benefits marginally from the multi-task setting
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diff changeset
784 in the case of digits (5\% relative improvement) but is actually hurt in the case
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785 of characters (respectively 3\% and 4\% worse for lower and upper class characters).
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786 On the other hand the SDA benefitted from the multi-task setting, with relative
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diff changeset
787 error rate improvements of 27\%, 15\% and 13\% respectively for digits,
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parents: 458
diff changeset
788 lower and upper case characters, as shown in Table~\ref{tab:multi-task}.
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diff changeset
789
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790 \begin{table}
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791 \caption{Test error rates and relative change in error rates due to the use of
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792 a multi-task setting, i.e., training on each task in isolation vs training
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793 for all three tasks together, for MLPs vs SDAs. The SDA benefits much
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794 more from the multi-task setting. All experiments on only on the
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diff changeset
795 unperturbed NIST data, using validation error for model selection.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
796 Relative improvement is 1 - single-task error / multi-task error.}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
797 \label{tab:multi-task}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
798 \begin{center}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
799 \begin{tabular}{|l|r|r|r|} \hline
fe292653a0f8 ajoute dernier tableau de resultats
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
800 & single-task & multi-task & relative \\
fe292653a0f8 ajoute dernier tableau de resultats
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
801 & setting & setting & improvement \\ \hline
fe292653a0f8 ajoute dernier tableau de resultats
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
802 MLP-digits & 3.77\% & 3.99\% & 5.6\% \\ \hline
fe292653a0f8 ajoute dernier tableau de resultats
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
803 MLP-lower & 17.4\% & 16.8\% & -4.1\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
804 MLP-upper & 7.84\% & 7.54\% & -3.6\% \\ \hline
fe292653a0f8 ajoute dernier tableau de resultats
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
805 SDA-digits & 2.6\% & 3.56\% & 27\% \\ \hline
fe292653a0f8 ajoute dernier tableau de resultats
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
806 SDA-lower & 12.3\% & 14.4\% & 15\% \\ \hline
fe292653a0f8 ajoute dernier tableau de resultats
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
807 SDA-upper & 5.93\% & 6.78\% & 13\% \\ \hline
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
808 \end{tabular}
fe292653a0f8 ajoute dernier tableau de resultats
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
809 \end{center}
fe292653a0f8 ajoute dernier tableau de resultats
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 458
diff changeset
810 \end{table}
437
479f2f518fc9 added Training with More Classes than Necessary
Guillaume Sicard <guitch21@gmail.com>
parents: 434
diff changeset
811
379
a21a174c1c18 added writeup skeleton
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
812 \section{Conclusions}
a21a174c1c18 added writeup skeleton
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
813
407
fe2e2964e7a3 description des transformations en cours ajout d un fichier special.bib pour des references specifiques
Xavier Glorot <glorotxa@iro.umontreal.ca>
parents: 393
diff changeset
814 \bibliography{strings,ml,aigaion,specials}
379
a21a174c1c18 added writeup skeleton
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
815 \bibliographystyle{mlapa}
a21a174c1c18 added writeup skeleton
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
816
407
fe2e2964e7a3 description des transformations en cours ajout d un fichier special.bib pour des references specifiques
Xavier Glorot <glorotxa@iro.umontreal.ca>
parents: 393
diff changeset
817 \end{document}