annotate writeup/nips2010_submission.tex @ 483:b9cdb464de5f

pointeur a la demo
author Yoshua Bengio <bengioy@iro.umontreal.ca>
date Mon, 31 May 2010 17:57:45 -0400
parents ce69aa9204d8
children 9a757d565e46
rev   line source
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1 \documentclass{article} % For LaTeX2e
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2 \usepackage{nips10submit_e,times}
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3
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4 \usepackage{amsthm,amsmath,amssymb,bbold,bbm}
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5 \usepackage{algorithm,algorithmic}
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6 \usepackage[utf8]{inputenc}
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7 \usepackage{graphicx,subfigure}
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8 \usepackage[numbers]{natbib}
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9
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10 \title{Deep Self-Taught Learning for Handwritten Character Recognition}
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11 \author{The IFT6266 Gang}
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12
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13 \begin{document}
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14
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15 %\makeanontitle
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16 \maketitle
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17
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18 \begin{abstract}
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19 Recent theoretical and empirical work in statistical machine learning has
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20 demonstrated the importance of learning algorithms for deep
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21 architectures, i.e., function classes obtained by composing multiple
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22 non-linear transformations. The self-taught learning (exploitng unlabeled
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23 examples or examples from other distributions) has already been applied
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24 to deep learners, but mostly to show the advantage of unlabeled
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25 examples. Here we explore the advantage brought by {\em out-of-distribution
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26 examples} and show that {\em deep learners benefit more from them than a
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27 corresponding shallow learner}, in the area
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28 of handwritten character recognition. In fact, we show that they reach
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29 human-level performance on both handwritten digit classification and
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30 62-class handwritten character recognition. For this purpose we
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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31 developed a powerful generator of stochastic variations and noise
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32 processes character images, including not only affine transformations but
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33 also slant, local elastic deformations, changes in thickness, background
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34 images, color, contrast, occlusion, and various types of pixel and
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35 spatially correlated noise. The out-of-distribution examples are
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36 obtained by training with these highly distorted images or
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37 by including object classes different from those in the target test set.
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38 \end{abstract}
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39
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40 \section{Introduction}
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41
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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42 Deep Learning has emerged as a promising new area of research in
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43 statistical machine learning (see~\citet{Bengio-2009} for a review).
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44 Learning algorithms for deep architectures are centered on the learning
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45 of useful representations of data, which are better suited to the task at hand.
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46 This is in great part inspired by observations of the mammalian visual cortex,
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47 which consists of a chain of processing elements, each of which is associated with a
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48 different representation. In fact,
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49 it was found recently that the features learnt in deep architectures resemble
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50 those observed in the first two of these stages (in areas V1 and V2
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51 of visual cortex)~\citep{HonglakL2008}.
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52 Processing images typically involves transforming the raw pixel data into
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53 new {\bf representations} that can be used for analysis or classification.
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54 For example, a principal component analysis representation linearly projects
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55 the input image into a lower-dimensional feature space.
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56 Why learn a representation? Current practice in the computer vision
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57 literature converts the raw pixels into a hand-crafted representation
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58 e.g.\ SIFT features~\citep{Lowe04}, but deep learning algorithms
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59 tend to discover similar features in their first few
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60 levels~\citep{HonglakL2008,ranzato-08,Koray-08,VincentPLarochelleH2008-very-small}.
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61 Learning increases the
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62 ease and practicality of developing representations that are at once
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63 tailored to specific tasks, yet are able to borrow statistical strength
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64 from other related tasks (e.g., modeling different kinds of objects). Finally, learning the
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65 feature representation can lead to higher-level (more abstract, more
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66 general) features that are more robust to unanticipated sources of
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67 variance extant in real data.
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68
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69 Whereas a deep architecture can in principle be more powerful than a
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70 shallow one in terms of representation, depth appears to render the
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71 training problem more difficult in terms of optimization and local minima.
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72 It is also only recently that successful algorithms were proposed to
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73 overcome some of these difficulties. All are based on unsupervised
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74 learning, often in an greedy layer-wise ``unsupervised pre-training''
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75 stage~\citep{Bengio-2009}. One of these layer initialization techniques,
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76 applied here, is the Denoising
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77 Auto-Encoder~(DEA)~\citep{VincentPLarochelleH2008-very-small}, which
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78 performed similarly or better than previously proposed Restricted Boltzmann
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79 Machines in terms of unsupervised extraction of a hierarchy of features
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80 useful for classification. The principle is that each layer starting from
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81 the bottom is trained to encode their input (the output of the previous
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82 layer) and try to reconstruct it from a corrupted version of it. After this
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83 unsupervised initialization, the stack of denoising auto-encoders can be
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84 converted into a deep supervised feedforward neural network and trained by
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85 stochastic gradient descent.
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86
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87 In this paper we ask the following questions:
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88 \begin{enumerate}
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89 \item Do the good results previously obtained with deep architectures on the
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90 MNIST digits generalize to the setting of a much larger and richer (but similar)
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91 dataset, the NIST special database 19, with 62 classes and around 800k examples?
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92 \item To what extent does the perturbation of input images (e.g. adding
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93 noise, affine transformations, background images) make the resulting
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94 classifier better not only on similarly perturbed images but also on
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95 the {\em original clean examples}?
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96 \item Do deep architectures benefit more from such {\em out-of-distribution}
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97 examples, i.e. do they benefit more from the self-taught learning~\citep{RainaR2007} framework?
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98 \item Similarly, does the feature learning step in deep learning algorithms benefit more
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99 training with similar but different classes (i.e. a multi-task learning scenario) than
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100 a corresponding shallow and purely supervised architecture?
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101 \end{enumerate}
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102 The experimental results presented here provide positive evidence towards all of these questions.
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103
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104 \section{Perturbation and Transformation of Character Images}
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105
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106 This section describes the different transformations we used to stochastically
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107 transform source images in order to obtain data. More details can
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108 be found in this technical report~\citep{ift6266-tr-anonymous}.
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109 The code for these transformations (mostly python) is available at
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110 {\tt http://anonymous.url.net}. All the modules in the pipeline share
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111 a global control parameter ($0 \le complexity \le 1$) that allows one to modulate the
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112 amount of deformation or noise introduced.
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113
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114 There are two main parts in the pipeline. The first one,
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115 from slant to pinch below, performs transformations. The second
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116 part, from blur to contrast, adds different kinds of noise.
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117
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118 {\large\bf Transformations}\\
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119
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120 {\bf Slant.}
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121 We mimic slant by shifting each row of the image
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122 proportionnaly to its height: $shift = round(slant \times height)$.
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123 The $slant$ coefficient can be negative or positive with equal probability
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124 and its value is randomly sampled according to the complexity level:
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125 e $slant \sim U[0,complexity]$, so the
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126 maximum displacement for the lowest or highest pixel line is of
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127 $round(complexity \times 32)$.\\
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128 {\bf Thickness.}
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129 Morpholigical 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
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
134 increasing dimensions (largest is $5\times5$) were used. For each image,
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
135 randomly sample the operator type (dilation or erosion) with equal probability and one structural
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
136 element from a subset of the $n$ smallest structuring elements where $n$ is
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
137 $round(10 \times complexity)$ for dilation and $round(6 \times complexity)$
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
138 for erosion. A neutral element is always present in the set, and if it is
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
139 chosen no transformation is applied. Erosion allows only the six
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
140 smallest structural elements because when the character is too thin it may
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
141 be completely erased.\\
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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142 {\bf Affine Transformations.}
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
143 A $2 \times 3$ affine transform matrix (with
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
144 6 parameters $(a,b,c,d,e,f)$) is sampled according to the $complexity$ level.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
145 Each pixel $(x,y)$ of the output image takes the value of the pixel
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
146 nearest to $(ax+by+c,dx+ey+f)$ in the input image. This
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
147 produces scaling, translation, rotation and shearing.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
148 The marginal distributions of $(a,b,c,d,e,f)$ have been tuned by hand to
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
149 forbid important rotations (not to confuse classes) but to give good
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
150 variability of the transformation: $a$ and $d$ $\sim U[1-3 \times
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
151 complexity,1+3 \times complexity]$, $b$ and $e$ $\sim[-3 \times complexity,3
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
152 \times complexity]$ and $c$ and $f$ $\sim U[-4 \times complexity, 4 \times
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
153 complexity]$.\\
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 472
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154 {\bf Local Elastic Deformations.}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 467
diff changeset
155 This filter induces a "wiggly" effect in the image, following~\citet{SimardSP03},
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
156 which provides more details.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
157 Two "displacements" fields are generated and applied, for horizontal
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
158 and vertical displacements of pixels.
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
159 To generate a pixel in either field, first a value between -1 and 1 is
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
160 chosen from a uniform distribution. Then all the pixels, in both fields, are
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
161 multiplied by a constant $\alpha$ which controls the intensity of the
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
162 displacements (larger $\alpha$ translates into larger wiggles).
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
163 Each field is convoluted with a Gaussian 2D kernel of
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
164 standard deviation $\sigma$. Visually, this results in a blur.
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
165 $\alpha = \sqrt[3]{complexity} \times 10.0$ and $\sigma = 10 - 7 \times
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
166 \sqrt[3]{complexity}$.\\
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 472
diff changeset
167 {\bf Pinch.}
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
168 This GIMP filter is named "Whirl and
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
169 pinch", but whirl was set to 0. A pinch is ``similar to projecting the image onto an elastic
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 467
diff changeset
170 surface and pressing or pulling on the center of the surface''~\citep{GIMP-manual}.
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
171 For a square input image, think of drawing a circle of
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
172 radius $r$ around a center point $C$. Any point (pixel) $P$ belonging to
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
173 that disk (region inside circle) will have its value recalculated by taking
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
174 the value of another "source" pixel in the original image. The position of
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
175 that source pixel is found on the line thats goes through $C$ and $P$, but
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
176 at some other distance $d_2$. Define $d_1$ to be the distance between $P$
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
177 and $C$. $d_2$ is given by $d_2 = sin(\frac{\pi{}d_1}{2r})^{-pinch} \times
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
178 d_1$, where $pinch$ is a parameter to the filter.
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
179 The actual value is given by bilinear interpolation considering the pixels
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
180 around the (non-integer) source position thus found.
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
181 Here $pinch \sim U[-complexity, 0.7 \times complexity]$.\\
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
182
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
183 {\large\bf Injecting Noise}\\
483
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 482
diff changeset
184
474
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 472
diff changeset
185 {\bf Motion Blur.}
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
186 This GIMP filter is a ``linear motion blur'' in GIMP
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
187 terminology, with two parameters, $length$ and $angle$. The value of
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
188 a pixel in the final image is the approximately mean value of the $length$ first pixels
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
189 found by moving in the $angle$ direction.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
190 Here $angle \sim U[0,360]$ degrees, and $length \sim {\rm Normal}(0,(3 \times complexity)^2)$.\\
474
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 472
diff changeset
191 {\bf Occlusion.}
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
192 This filter selects a random rectangle from an {\em occluder} character
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
193 images and places it over the original {\em occluded} character
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
194 image. Pixels are combined by taking the max(occluder,occluded),
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
195 closer to black. The corners of the occluder The rectangle corners
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
196 are sampled so that larger complexity gives larger rectangles.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
197 The destination position in the occluded image are also sampled
469
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 467
diff changeset
198 according to a normal distribution (see more details in~\citet{ift6266-tr-anonymous}).
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
199 It has has a probability of not being applied at all of 60\%.\\
474
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 472
diff changeset
200 {\bf Pixel Permutation.}
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
201 This filter permutes neighbouring pixels. It selects first
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
202 $\frac{complexity}{3}$ pixels randomly in the image. Each of them are then
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
203 sequentially exchanged to one other pixel in its $V4$ neighbourhood. Number
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
204 of exchanges to the left, right, top, bottom are equal or does not differ
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
205 from more than 1 if the number of selected pixels is not a multiple of 4.
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
206 It has has a probability of not being applied at all of 80\%.\\
474
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 472
diff changeset
207 {\bf Gaussian Noise.}
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
208 This filter simply adds, to each pixel of the image independently, a
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
209 noise $\sim Normal(0(\frac{complexity}{10})^2)$.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
210 It has has a probability of not being applied at all of 70\%.\\
474
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 472
diff changeset
211 {\bf Background Images.}
469
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 467
diff changeset
212 Following~\citet{Larochelle-jmlr-2009}, this transformation adds a random
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
213 background behind the letter. The background is chosen by first selecting,
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
214 at random, an image from a set of images. Then a 32$\times$32 subregion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
215 of that image is chosen as the background image (by sampling position
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
216 uniformly while making sure not to cross image borders).
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
217 To combine the original letter image and the background image, contrast
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
218 adjustments are made. We first get the maximal values (i.e. maximal
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
219 intensity) for both the original image and the background image, $maximage$
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
220 and $maxbg$. We also have a parameter $contrast \sim U[complexity, 1]$.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
221 Each background pixel value is multiplied by $\frac{max(maximage -
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
222 contrast, 0)}{maxbg}$ (higher contrast yield darker
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
223 background). The output image pixels are max(background,original).\\
474
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 472
diff changeset
224 {\bf Salt and Pepper Noise.}
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
225 This filter adds noise $\sim U[0,1]$ to random subsets of pixels.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
226 The number of selected pixels is $0.2 \times complexity$.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
227 This filter has a probability of not being applied at all of 75\%.\\
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 472
diff changeset
228 {\bf Spatially Gaussian Noise.}
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
229 Different regions of the image are spatially smoothed.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
230 The image is convolved with a symmetric Gaussian kernel of
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
231 size and variance choosen uniformly in the ranges $[12,12 + 20 \times
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
232 complexity]$ and $[2,2 + 6 \times complexity]$. The result is normalized
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
233 between $0$ and $1$. We also create a symmetric averaging window, of the
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
234 kernel size, with maximum value at the center. For each image we sample
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
235 uniformly from $3$ to $3 + 10 \times complexity$ pixels that will be
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
236 averaging centers between the original image and the filtered one. We
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
237 initialize to zero a mask matrix of the image size. For each selected pixel
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
238 we add to the mask the averaging window centered to it. The final image is
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
239 computed from the following element-wise operation: $\frac{image + filtered
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
240 image \times mask}{mask+1}$.
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
241 This filter has a probability of not being applied at all of 75\%.\\
474
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 472
diff changeset
242 {\bf Scratches.}
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
243 The scratches module places line-like white patches on the image. The
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
244 lines are heavily transformed images of the digit "1" (one), chosen
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
245 at random among five thousands such 1 images. The 1 image is
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
246 randomly cropped and rotated by an angle $\sim Normal(0,(100 \times
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
247 complexity)^2$, using bicubic interpolation,
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
248 Two passes of a greyscale morphological erosion filter
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
249 are applied, reducing the width of the line
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
250 by an amount controlled by $complexity$.
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
251 This filter is only applied only 15\% of the time. When it is applied, 50\%
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
252 of the time, only one patch image is generated and applied. In 30\% of
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
253 cases, two patches are generated, and otherwise three patches are
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
254 generated. The patch is applied by taking the maximal value on any given
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
255 patch or the original image, for each of the 32x32 pixel locations.\\
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 472
diff changeset
256 {\bf Color and Contrast Changes.}
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
257 This filter changes the constrast and may invert the image polarity (white
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
258 on black to black on white). The contrast $C$ is defined here as the
467
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
259 difference between the maximum and the minimum pixel value of the image.
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
260 Contrast $\sim U[1-0.85 \times complexity,1]$ (so constrast $\geq 0.15$).
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 466
diff changeset
261 The image is normalized into $[\frac{1-C}{2},1-\frac{1-C}{2}]$. The
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
262 polarity is inverted with $0.5$ probability.
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
263
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
264
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
265 \begin{figure}[h]
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
266 \resizebox{.99\textwidth}{!}{\includegraphics{images/example_t.png}}\\
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
267 \caption{Illustration of the pipeline of stochastic
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
268 transformations applied to the image of a lower-case t
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
269 (the upper left image). Each image in the pipeline (going from
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
270 left to right, first top line, then bottom line) shows the result
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
271 of applying one of the modules in the pipeline. The last image
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
272 (bottom right) is used as training example.}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
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273 \label{fig:pipeline}
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274 \end{figure}
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275
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276
479
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277 \begin{figure}[h]
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278 \resizebox{.99\textwidth}{!}{\includegraphics{images/transfo.png}}\\
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279 \caption{Illustration of each transformation applied alone to the same image
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280 of an upper-case h (top left). First row (from left to rigth) : original image, slant,
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281 thickness, affine transformation, local elastic deformation; second row (from left to rigth) :
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parents: 480
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282 pinch, motion blur, occlusion, pixel permutation, Gaussian noise; third row (from left to rigth) :
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283 background image, salt and pepper noise, spatially Gaussian noise, scratches,
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284 color and contrast changes.}
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285 \label{fig:transfo}
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286 \end{figure}
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287
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288
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289
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290 \section{Experimental Setup}
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291
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292 Whereas much previous work on deep learning algorithms had been performed on
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293 the MNIST digits classification task~\citep{Hinton06,ranzato-07,Bengio-nips-2006,Salakhutdinov+Hinton-2009},
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294 with 60~000 examples, and variants involving 10~000
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295 examples~\cite{Larochelle-jmlr-toappear-2008,VincentPLarochelleH2008}, we want
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296 to focus here on the case of much larger training sets, from 10 times to
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297 to 1000 times larger. The larger datasets are obtained by first sampling from
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298 a {\em data source} (NIST characters, scanned machine printed characters, characters
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Yoshua Bengio <bengioy@iro.umontreal.ca>
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299 from fonts, or characters from captchas) and then optionally applying some of the
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
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300 above transformations and/or noise processes.
464
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301
472
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302 \subsection{Data Sources}
464
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303
24f4a8b53fcc nips2010_submission.tex
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304 \begin{itemize}
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305 \item {\bf NIST}
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306 Our main source of characters is the NIST Special Database 19~\cite{Grother-1995},
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307 widely used for training and testing character
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308 recognition systems~\cite{Granger+al-2007,Cortes+al-2000,Oliveira+al-2002,Milgram+al-2005}.
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309 The dataset is composed with 8????? digits and characters (upper and lower cases), with hand checked classifications,
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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310 extracted from handwritten sample forms of 3600 writers. The characters are labelled by one of the 62 classes
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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311 corresponding to "0"-"9","A"-"Z" and "a"-"z". The dataset contains 8 series of different complexity.
472
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312 The fourth series, $hsf_4$, experimentally recognized to be the most difficult one is recommended
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parents: 469
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313 by NIST as testing set and is used in our work and some previous work~\cite{Granger+al-2007,Cortes+al-2000,Oliveira+al-2002,Milgram+al-2005}
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parents: 469
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314 for that purpose. We randomly split the remainder into a training set and a validation set for
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315 model selection. The sizes of these data sets are: 651668 for training, 80000 for validation,
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diff changeset
316 and 82587 for testing.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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317 The performances reported by previous work on that dataset mostly use only the digits.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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318 Here we use all the classes both in the training and testing phase. This is especially
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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319 useful to estimate the effect of a multi-task setting.
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
320 Note that the distribution of the classes in the NIST training and test sets differs
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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321 substantially, with relatively many more digits in the test set, and uniform distribution
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
322 of letters in the test set, not in the training set (more like the natural distribution
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
323 of letters in text).
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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324
479
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325 \item {\bf Fonts}
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parents: 476
diff changeset
326 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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parents: 476
diff changeset
327 %real adress {\tt http://cg.scs.carleton.ca/~luc/freefonts.html}
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parents: 476
diff changeset
328 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: 476
diff changeset
329 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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Xavier Glorot <glorotxa@iro.umontreal.ca>
parents: 476
diff changeset
330 directly as input to our models.
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parents: 476
diff changeset
331
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parents: 476
diff changeset
332
464
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
333
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
334 \item {\bf Captchas}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
335 The Captcha data source is an adaptation of the \emph{pycaptcha} library (a python based captcha generator library) for
472
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
336 generating characters of the same format as the NIST dataset. This software is based on
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
337 a random character class generator and various kinds of tranformations similar to those described in the previous sections.
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
338 In order to increase the variability of the data generated, many different fonts are used for generating the characters.
464
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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339 Transformations (slant, distorsions, rotation, translation) are applied to each randomly generated character with a complexity
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
340 depending on the value of the complexity parameter provided by the user of the data source. Two levels of complexity are
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
341 allowed and can be controlled via an easy to use facade class.
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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342 \item {\bf OCR data}
472
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
343 A large set (2 million) of scanned, OCRed and manually verified machine-printed
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
344 characters (from various documents and books) where included as an
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
345 additional source. This set is part of a larger corpus being collected by the Image Understanding
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
346 Pattern Recognition Research group lead by Thomas Breuel at University of Kaiserslautern
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
347 ({\tt http://www.iupr.com}), and which will be publically released.
464
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
348 \end{itemize}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
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349
472
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diff changeset
350 \subsection{Data Sets}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
351 All data sets contain 32$\times$32 grey-level images (values in $[0,1]$) associated with a label
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
352 from one of the 62 character classes.
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
353 \begin{itemize}
472
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parents: 469
diff changeset
354 \item {\bf NIST}. This is the raw NIST special database 19.
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
355 \item {\bf P07}. This dataset is obtained by taking raw characters from all four of the above sources
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
356 and sending them through the above transformation pipeline.
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
357 For each new exemple to generate, a source is selected with probability $10\%$ from the fonts,
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
358 $25\%$ from the captchas, $25\%$ from the OCR data and $40\%$ from NIST. We apply all the transformations in the
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
359 order given above, and for each of them we sample uniformly a complexity in the range $[0,0.7]$.
464
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
360 \item {\bf NISTP} NISTP is equivalent to P07 (complexity parameter of $0.7$ with the same sources proportion)
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
361 except that we only apply
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
362 transformations from slant to pinch. Therefore, the character is
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
363 transformed but no additionnal noise is added to the image, giving images
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
364 closer to the NIST dataset.
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
365 \end{itemize}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
366
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
367 \subsection{Models and their Hyperparameters}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
368
472
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
369 All hyper-parameters are selected based on performance on the NISTP validation set.
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parents: 469
diff changeset
370
464
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
371 \subsubsection{Multi-Layer Perceptrons (MLP)}
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
372
472
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
373 Whereas previous work had compared deep architectures to both shallow MLPs and
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
374 SVMs, we only compared to MLPs here because of the very large datasets used.
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
375 The MLP has a single hidden layer with $\tanh$ activation functions, and softmax (normalized
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
376 exponentials) on the output layer for estimating P(class | image).
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
377 The hyper-parameters are the following: number of hidden units, taken in
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
378 $\{300,500,800,1000,1500\}$. The optimization procedure is as follows. Training
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
379 examples are presented in minibatches of size 20. A constant learning
474
bcf024e6ab23 fits now, but still now graphics
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 472
diff changeset
380 rate is chosen in $10^{-3},0.01, 0.025, 0.075, 0.1, 0.5\}$
472
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
381 through preliminary experiments, and 0.1 was selected.
464
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
382
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
383
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
384 \subsubsection{Stacked Denoising Auto-Encoders (SDAE)}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
385 \label{SdA}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
386
472
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
387 Various auto-encoder variants and Restricted Boltzmann Machines (RBMs)
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
388 can be used to initialize the weights of each layer of a deep MLP (with many hidden
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
389 layers)~\citep{Hinton06,ranzato-07,Bengio-nips-2006}
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
390 enabling better generalization, apparently setting parameters in the
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
391 basin of attraction of supervised gradient descent yielding better
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
392 generalization~\citep{Erhan+al-2010}. It is hypothesized that the
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
393 advantage brought by this procedure stems from a better prior,
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
394 on the one hand taking advantage of the link between the input
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
395 distribution $P(x)$ and the conditional distribution of interest
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
396 $P(y|x)$ (like in semi-supervised learning), and on the other hand
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
397 taking advantage of the expressive power and bias implicit in the
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
398 deep architecture (whereby complex concepts are expressed as
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
399 compositions of simpler ones through a deep hierarchy).
464
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
400
472
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Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
401 Here we chose to use the Denoising
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
402 Auto-Encoder~\citep{VincentPLarochelleH2008} as the building block for
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
403 these deep hierarchies of features, as it is very simple to train and
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
404 teach (see tutorial and code there: {\tt http://deeplearning.net/tutorial}),
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
405 provides immediate and efficient inference, and yielded results
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
406 comparable or better than RBMs in series of experiments
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
407 \citep{VincentPLarochelleH2008}. During training of a Denoising
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
408 Auto-Encoder, it is presented with a stochastically corrupted version
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
409 of the input and trained to reconstruct the uncorrupted input,
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
410 forcing the hidden units to represent the leading regularities in
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
411 the data. Once it is trained, its hidden units activations can
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
412 be used as inputs for training a second one, etc.
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
413 After this unsupervised pre-training stage, the parameters
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
414 are used to initialize a deep MLP, which is fine-tuned by
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
415 the same standard procedure used to train them (see previous section).
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
416
472
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
417 The hyper-parameters are the same as for the MLP, with the addition of the
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
418 amount of corruption noise (we used the masking noise process, whereby a
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
419 fixed proportion of the input values, randomly selected, are zeroed), and a
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
420 separate learning rate for the unsupervised pre-training stage (selected
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
421 from the same above set). The fraction of inputs corrupted was selected
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
422 among $\{10\%, 20\%, 50\%\}$. Another hyper-parameter is the number
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
423 of hidden layers but it was fixed to 3 based on previous work with
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
424 stacked denoising auto-encoders on MNIST~\citep{VincentPLarochelleH2008}.
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
425
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
426 \section{Experimental Results}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
427
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
428 \subsection{SDA vs MLP vs Humans}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
429
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
430 We compare here the best MLP (according to validation set error) that we found against
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
431 the best SDA (again according to validation set error), along with a precise estimate
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
432 of human performance obtained via Amazon's Mechanical Turk (AMT)
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
433 service\footnote{http://mturk.com}. AMT users are paid small amounts
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
434 of money to perform tasks for which human intelligence is required.
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
435 Mechanical Turk has been used extensively in natural language
469
d02d288257bf redone bib style
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 467
diff changeset
436 processing \citep{SnowEtAl2008} and vision
d02d288257bf redone bib style
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 467
diff changeset
437 \citep{SorokinAndForsyth2008,whitehill09}. AMT users where presented
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
438 with 10 character images and asked to type 10 corresponding ascii
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
439 characters. Hence they were forced to make a hard choice among the
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
440 62 character classes. Three users classified each image, allowing
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
441 to estimate inter-human variability (shown as +/- in parenthesis below).
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
442
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
443 \begin{table}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
444 \caption{Overall comparison of error rates ($\pm$ std.err.) on 62 character classes (10 digits +
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
445 26 lower + 26 upper), except for last columns -- digits only, between deep architecture with pre-training
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
446 (SDA=Stacked Denoising Autoencoder) and ordinary shallow architecture
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
447 (MLP=Multi-Layer Perceptron). The models shown are all trained using perturbed data (NISTP or P07)
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
448 and using a validation set to select hyper-parameters and other training choices.
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
449 \{SDA,MLP\}0 are trained on NIST,
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
450 \{SDA,MLP\}1 are trained on NISTP, and \{SDA,MLP\}2 are trained on P07.
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
451 The human error rate on digits is a lower bound because it does not count digits that were
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
452 recognized as letters. For comparison, the results found in the literature
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
453 on NIST digits classification using the same test set are included.}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
454 \label{tab:sda-vs-mlp-vs-humans}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
455 \begin{center}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
456 \begin{tabular}{|l|r|r|r|r|} \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
457 & NIST test & NISTP test & P07 test & NIST test digits \\ \hline
472
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
458 Humans& 18.2\% $\pm$.1\% & 39.4\%$\pm$.1\% & 46.9\%$\pm$.1\% & $1.4\%$ \\ \hline
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
459 SDA0 & 23.7\% $\pm$.14\% & 65.2\%$\pm$.34\% & 97.45\%$\pm$.06\% & 2.7\% $\pm$.14\%\\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
460 SDA1 & 17.1\% $\pm$.13\% & 29.7\%$\pm$.3\% & 29.7\%$\pm$.3\% & 1.4\% $\pm$.1\%\\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
461 SDA2 & 18.7\% $\pm$.13\% & 33.6\%$\pm$.3\% & 39.9\%$\pm$.17\% & 1.7\% $\pm$.1\%\\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
462 MLP0 & 24.2\% $\pm$.15\% & 68.8\%$\pm$.33\% & 78.70\%$\pm$.14\% & 3.45\% $\pm$.15\% \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
463 MLP1 & 23.0\% $\pm$.15\% & 41.8\%$\pm$.35\% & 90.4\%$\pm$.1\% & 3.85\% $\pm$.16\% \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
464 MLP2 & 24.3\% $\pm$.15\% & 46.0\%$\pm$.35\% & 54.7\%$\pm$.17\% & 4.85\% $\pm$.18\% \\ \hline
469
d02d288257bf redone bib style
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 467
diff changeset
465 \citep{Granger+al-2007} & & & & 4.95\% $\pm$.18\% \\ \hline
d02d288257bf redone bib style
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 467
diff changeset
466 \citep{Cortes+al-2000} & & & & 3.71\% $\pm$.16\% \\ \hline
d02d288257bf redone bib style
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 467
diff changeset
467 \citep{Oliveira+al-2002} & & & & 2.4\% $\pm$.13\% \\ \hline
472
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
468 \citep{Milgram+al-2005} & & & & 2.1\% $\pm$.12\% \\ \hline
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
469 \end{tabular}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
470 \end{center}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
471 \end{table}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
472
475
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
473 \begin{figure}[h]
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
474 \resizebox{.99\textwidth}{!}{\includegraphics{images/error_rates_charts.pdf}}\\
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
475 \caption{Charts corresponding to table \ref{tab:sda-vs-mlp-vs-humans}. Left: overall results; error bars indicate a 95\% confidence interval. Right: error rates on NIST test digits only, with results from litterature. }
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
476 \label{fig:error-rates-charts}
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
477 \end{figure}
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
478
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
479 \subsection{Perturbed Training Data More Helpful for SDAE}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
480
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
481 \begin{table}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
482 \caption{Relative change in error rates due to the use of perturbed training data,
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
483 either using NISTP, for the MLP1/SDA1 models, or using P07, for the MLP2/SDA2 models.
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
484 A positive value indicates that training on the perturbed data helped for the
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
485 given test set (the first 3 columns on the 62-class tasks and the last one is
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
486 on the clean 10-class digits). Clearly, the deep learning models did benefit more
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
487 from perturbed training data, even when testing on clean data, whereas the MLP
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
488 trained on perturbed data performed worse on the clean digits and about the same
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
489 on the clean characters. }
469
d02d288257bf redone bib style
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 467
diff changeset
490 \label{tab:perturbation-effect}
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
491 \begin{center}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
492 \begin{tabular}{|l|r|r|r|r|} \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
493 & NIST test & NISTP test & P07 test & NIST test digits \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
494 SDA0/SDA1-1 & 38\% & 84\% & 228\% & 93\% \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
495 SDA0/SDA2-1 & 27\% & 94\% & 144\% & 59\% \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
496 MLP0/MLP1-1 & 5.2\% & 65\% & -13\% & -10\% \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
497 MLP0/MLP2-1 & -0.4\% & 49\% & 44\% & -29\% \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
498 \end{tabular}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
499 \end{center}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
500 \end{table}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
501
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
502
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
503 \subsection{Multi-Task Learning Effects}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
504
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
505 As previously seen, the SDA is better able to benefit from the
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
506 transformations applied to the data than the MLP. In this experiment we
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
507 define three tasks: recognizing digits (knowing that the input is a digit),
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
508 recognizing upper case characters (knowing that the input is one), and
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
509 recognizing lower case characters (knowing that the input is one). We
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
510 consider the digit classification task as the target task and we want to
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
511 evaluate whether training with the other tasks can help or hurt, and
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
512 whether the effect is different for MLPs versus SDAs. The goal is to find
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
513 out if deep learning can benefit more (or less) from multiple related tasks
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
514 (i.e. the multi-task setting) compared to a corresponding purely supervised
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
515 shallow learner.
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
516
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
517 We use a single hidden layer MLP with 1000 hidden units, and a SDA
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
518 with 3 hidden layers (1000 hidden units per layer), pre-trained and
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
519 fine-tuned on NIST.
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
520
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
521 Our results show that the MLP benefits marginally from the multi-task setting
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
522 in the case of digits (5\% relative improvement) but is actually hurt in the case
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
523 of characters (respectively 3\% and 4\% worse for lower and upper class characters).
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
524 On the other hand the SDA benefitted from the multi-task setting, with relative
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
525 error rate improvements of 27\%, 15\% and 13\% respectively for digits,
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
526 lower and upper case characters, as shown in Table~\ref{tab:multi-task}.
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
527
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
528 \begin{table}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
529 \caption{Test error rates and relative change in error rates due to the use of
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
530 a multi-task setting, i.e., training on each task in isolation vs training
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
531 for all three tasks together, for MLPs vs SDAs. The SDA benefits much
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
532 more from the multi-task setting. All experiments on only on the
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
533 unperturbed NIST data, using validation error for model selection.
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
534 Relative improvement is 1 - single-task error / multi-task error.}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
535 \label{tab:multi-task}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
536 \begin{center}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
537 \begin{tabular}{|l|r|r|r|} \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
538 & single-task & multi-task & relative \\
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
539 & setting & setting & improvement \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
540 MLP-digits & 3.77\% & 3.99\% & 5.6\% \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
541 MLP-lower & 17.4\% & 16.8\% & -4.1\% \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
542 MLP-upper & 7.84\% & 7.54\% & -3.6\% \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
543 SDA-digits & 2.6\% & 3.56\% & 27\% \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
544 SDA-lower & 12.3\% & 14.4\% & 15\% \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
545 SDA-upper & 5.93\% & 6.78\% & 13\% \\ \hline
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
546 \end{tabular}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
547 \end{center}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
548 \end{table}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
549
475
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
550
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
551 \begin{figure}[h]
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
552 \resizebox{.99\textwidth}{!}{\includegraphics{images/improvements_charts.pdf}}\\
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
553 \caption{Charts corresponding to tables \ref{tab:perturbation-effect} (left) and \ref{tab:multi-task} (right).}
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
554 \label{fig:improvements-charts}
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
555 \end{figure}
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
556
483
b9cdb464de5f pointeur a la demo
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 482
diff changeset
557 A Flash demo of the recognizer (where both the MLP and the SDA can be compared)
b9cdb464de5f pointeur a la demo
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 482
diff changeset
558 can be executed on-line at {\tt http://deep.host22.com}.
475
ead3085c1c66 Added charts to nips2010_submission.tex
fsavard
parents: 469
diff changeset
559
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
560 \section{Conclusions}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
561
472
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
562 The conclusions are positive for all the questions asked in the introduction.
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
563 \begin{itemize}
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
564 \item Do the good results previously obtained with deep architectures on the
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
565 MNIST digits generalize to the setting of a much larger and richer (but similar)
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
566 dataset, the NIST special database 19, with 62 classes and around 800k examples?
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
567 Yes, the SDA systematically outperformed the MLP, in fact reaching human-level
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
568 performance.
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
569 \item To what extent does the perturbation of input images (e.g. adding
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
570 noise, affine transformations, background images) make the resulting
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
571 classifier better not only on similarly perturbed images but also on
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
572 the {\em original clean examples}? Do deep architectures benefit more from such {\em out-of-distribution}
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
573 examples, i.e. do they benefit more from the self-taught learning~\citep{RainaR2007} framework?
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
574 MLPs were helped by perturbed training examples when tested on perturbed input images,
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
575 but only marginally helped wrt clean examples. On the other hand, the deep SDAs
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
576 were very significantly boosted by these out-of-distribution examples.
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
577 \item Similarly, does the feature learning step in deep learning algorithms benefit more
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
578 training with similar but different classes (i.e. a multi-task learning scenario) than
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
579 a corresponding shallow and purely supervised architecture?
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
580 Whereas the improvement due to the multi-task setting was marginal or
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
581 negative for the MLP, it was very significant for the SDA.
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
582 \end{itemize}
2dd6e8962df1 conclusion
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 469
diff changeset
583
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
584 \bibliography{strings,ml,aigaion,specials}
469
d02d288257bf redone bib style
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 467
diff changeset
585 %\bibliographystyle{plainnat}
d02d288257bf redone bib style
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents: 467
diff changeset
586 \bibliographystyle{unsrtnat}
464
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
587 %\bibliographystyle{apalike}
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
588
24f4a8b53fcc nips2010_submission.tex
Yoshua Bengio <bengioy@iro.umontreal.ca>
parents:
diff changeset
589 \end{document}