MERL – A MITSUBISHI ELECTRIC RESEARCH LABORATORY
Rapid Object Detection Using a Boosted
Cascade of Simple Features
Paul Viola and Michael Jones
TR-2004-043 May 2004
This paper describes a machine learning approach for visual object detection which is capable
of processing images extremely rapidly and achieving high detection rates. This work is distin-
guished by three key contributions. The ﬁrst is the introduction of a new image representation
called the Integral Image which allows the features used by our detector to be computed very
quickly. The second is a learning algorithm, based on AdaBoost, which selects a small num-
ber of critical visual features from a larger set and yields extremely efﬁcient classiﬁers. The
third contribution is a method for combining increasingly more complex classiﬁers in a cascade
which allows background regions of the image to be quickly discarded while spending more
computation on promising object-like regions. The cascade can be viewed as an object speciﬁc
focus-of-attention mechanism which unlike previous approaches provides statistical guarantees
that discarded regions are unlikely to contain the object of interest. In the domain of face detec-
tion the system yields detection rates comparable to the best previous systems. Used in real-time
applications, the detector runs at 15 frames per second without resorting to image differencing
or skin color detection.
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Mitsubishi Electric Research Laboratories, Inc., 2004
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1. First printing, TR-2004-043, May 2004
ACCEPTED CONFERENCE ON COMPUTER VISION AND PATTERN RECOGNITION 2001
Rapid Object Detection using a Boosted Cascade of Simple
Paul Viola Michael Jones
Mitsubishi Electric Research Labs Compaq CRL
201 Broadway, 8th FL One Cambridge Center
Cambridge, MA 02139 Cambridge, MA 02142
This paper describes a machine learning approach for vi-
sual object detection which is capable of processing images
extremely rapidly and achieving high detection rates. This
work is distinguished by three key contributions. The ﬁrst
is the introduction of a new image representation called the
“Integral Image” which allows the features used by our de-
tector to be computed very quickly. The second is a learning
algorithm, based on AdaBoost, which selects a small num-
ber of critical visual features from a larger set and yields
extremely efﬁcient classiﬁers. The third contribution is
a method for combining increasingly more complex classi-
ﬁersin a “cascade” whichallowsbackground regions of the
image to be quickly discarded while spending more compu-
tation on promising object-like regions. The cascade can be
viewed as an object speciﬁc focus-of-attention mechanism
which unlike previous approaches provides statistical guar-
antees that discardedregions are unlikely to contain the ob-
ject of interest. In the domain of face detection the system
yields detection rates comparable to the best previous sys-
tems. Used in real-time applications, the detector runs at
15 frames per second without resorting to image differenc-
ing or skin color detection.
This paper brings together new algorithms and insights to
constructa frameworkfor robust and extremely rapid object
detection. This framework is demonstrated on, and in part
motivated by, the task of face detection. Toward this end
we have constructed a frontal face detection system which
achieves detection and false positive rates which are equiv-
alent to the best published results [16, 12, 15, 11, 1]. This
face detection system is most clearly distinguished from
previous approaches in its ability to detect faces extremely
rapidly. Operatingon384by288pixel images, faces are de-
tected at 15 frames per second on a conventional 700 MHz
Intel Pentium III. In other face detection systems, auxiliary
information, such as image differences in video sequences,
or pixel color in color images, have been used to achieve
high frame rates. Our system achieves high frame rates
working only with the information present in a single grey
scale image. These alternative sources of information can
also be integrated with our system to achieve even higher
There are three main contributions of our object detec-
tion framework. We will introduce each of these ideas
brieﬂy below and then describe them in detail in subsequent
The ﬁrst contribution of this paper is a new image repre-
sentation called an integral image that allows for very fast
feature evaluation. Motivated in part by the work of Papa-
georgiou et al. our detection system does not work directly
with image intensities . Like these authors we use a
set of features which are reminiscent of Haar Basis func-
tions (though we will also use related ﬁlters which are more
complex than Haar ﬁlters). In order to compute these fea-
tures very rapidly at many scales we introduce the integral
image representation for images. The integral image can be
computed from an image using a few operations per pixel.
Once computed, any one of these Harr-like features can be
computed at any scale or location in constant time.
The second contribution of this paper is a method for
constructing a classiﬁer by selecting a small number of im-
portant features using AdaBoost . Within any image sub-
window the total number of Harr-like features is very large,
far larger than the number of pixels. In order to ensure fast
classiﬁcation, the learning process must excludea largema-
jority of the available features, and focus on a small set of
critical features. Motivated by the work of Tieu and Viola,
feature selection is achieved through a simple modiﬁcation
of the AdaBoost procedure: the weak learner is constrained
so that each weak classiﬁer returned can depend on only a
single feature . As a result each stage of the boosting
process, which selects a new weak classiﬁer, can be viewed
as a feature selection process. AdaBoost provides an effec-
tive learning algorithm and strong bounds on generalization
performance [13, 9, 10].
The third major contribution of this paper is a method
for combining successively more complex classiﬁers in a
cascade structure which dramatically increases the speed of
the detector by focusing attention on promising regions of
the image. The notion behind focus of attention approaches
is that it is often possible to rapidly determine where in an
image an object might occur [17, 8, 1]. More complex pro-
cessing is reserved only for these promising regions. The
keymeasure of such an approach is the “false negative” rate
of the attentional process. It must be the case that all, or
almost all, object instances are selected by the attentional
We will describe a process for training an extremely sim-
ple and efﬁcient classiﬁer which can be used as a “super-
vised” focus of attention operator. The term supervised
refers to the fact that the attentional operator is trained to
detect examples of a particular class. In the domain of face
detection it is possible to achieve fewer than 1% false neg-
atives and 40% false positives using a classiﬁer constructed
from two Harr-like features. The effect of this ﬁlter is to
reduce by over one half the number of locations where the
ﬁnal detector must be evaluated.
Those sub-windows which are not rejected by the initial
classiﬁer are processed by a sequence of classiﬁers, each
slightly more complex than the last. If any classiﬁer rejects
the sub-window, no further processing is performed. The
structure of the cascaded detection process is essentially
that of a degenerate decision tree, and as such is related to
the work of Geman and colleagues [1, 4].
An extremely fast face detector will have broad prac-
tical applications. These include user interfaces, image
databases, and teleconferencing. In applications where
rapid frame-rates are not necessary, our system will allow
for signiﬁcant additional post-processing and analysis. In
addition our system can be implemented on a wide range of
small low power devices, including hand-helds and embed-
ded processors. In our lab we have implemented this face
detector on the Compaq iPaq handheld and have achieved
detection at two frames per second (this device has a low
power 200 mips Strong Arm processor which lacks ﬂoating
The remainder of the paper describes our contributions
and a number of experimental results, including a detailed
description of our experimental methodology. Discussion
of closely related work takes place at the end of each sec-
Our object detection procedure classiﬁes images based on
the value of simple features. There are many motivations
Figure 1: Example rectangle features shown relative to the
enclosing detection window. The sum of the pixels which
lie within the white rectangles are subtracted from the sum
of pixels in the grey rectangles. Two-rectangle features are
shown in (A) and (B). Figure (C) shows a three-rectangle
feature, and (D) a four-rectangle feature.
for using features rather than the pixels directly. The most
common reason is that features can act to encode ad-hoc
domain knowledge that is difﬁcult to learn using a ﬁnite
quantity of training data. For this system there is also a
second critical motivation for features: the feature based
system operates much faster than a pixel-based system.
The simple features used are reminiscent of Haar basis
functionswhichhavebeenused byPapageorgiouetal. .
More speciﬁcally, we use three kinds of features. The value
of a two-rectangle feature is the difference between the sum
of the pixels within two rectangular regions. The regions
have the same size and shape and are horizontally or ver-
tically adjacent (see Figure 1). A three-rectangle feature
computes the sum within two outside rectangles subtracted
from the sum in a center rectangle. Finally a four-rectangle
feature computes the difference between diagonal pairs of
Given that the base resolution of the detector is 24x24,
the exhaustive set of rectangle features is quite large, over
180,000 . Note that unlike the Haar basis, the set of rectan-
gle features is overcomplete
2.1. Integral Image
Rectangle features can be computed very rapidly using an
intermediate representation for the image which we call the
The integral image at location contains
the sum of the pixels above and to the left of , inclusive:
A complete basis has no linear dependence between basis elements
and has the same number of elements as the image space, in this case 576.
The full set of 180,000 thousand features is many times over-complete.
There is a close relation to “summed area tables” as used in graphics
. We choose a different name here in order to emphasize its use for the
analysis of images, rather than for texture mapping.
Figure 2: The sum of the pixels within rectangle can be
computed with four array references. The value of the inte-
gral image at location 1 is the sum of the pixels in rectangle
. The value at location 2 is , at location 3 is ,
and at location 4 is . The sum within can
be computed as .
where is the integral image and is the origi-
nal image. Using the following pair of recurrences:
is the cumulative row sum, ,
and ) the integral image can be computed in
one pass over the original image.
Using the integral image any rectangular sum can be
computed in four array references (see Figure 2). Clearly
the difference between two rectangular sums can be com-
puted in eight references. Since the two-rectangle features
deﬁned above involve adjacent rectangular sums they can
be computed in six array references, eight in the case of
the three-rectangle features, and nine for four-rectangle fea-
2.2. Feature Discussion
Rectangle features are somewhat primitive when compared
withalternatives such as steerable ﬁlters [5, 7]. Steerable ﬁl-
ters, and their relatives, are excellent for the detailed analy-
sis of boundaries, image compression, and texture analysis.
In contrast rectangle features, while sensitive to the pres-
ence of edges, bars, and other simple image structure, are
quite coarse. Unlike steerable ﬁlters the only orientations
available are vertical, horizontal, and diagonal. The set of
rectangle features do however provide a rich image repre-
sentation which supports effective learning. In conjunction
with the integral image , the efﬁciency of the rectangle fea-
ture set provides ample compensation for their limited ﬂex-
3. Learning Classiﬁcation Functions
Given a feature set and a training set of positive and neg-
ative images, any number of machine learning approaches
could be used to learn a classiﬁcation function. In our sys-
tem a variant of AdaBoost is used both to select a small set
of features and train the classiﬁer . In its original form,
the AdaBoost learning algorithm is used to boost the clas-
siﬁcation performance of a simple (sometimes called weak)
learning algorithm. There are a number of formal guaran-
tees provided by the AdaBoost learning procedure. Freund
and Schapire proved that the training error of the strong
classiﬁer approaches zero exponentially in the number of
rounds. More importantly a number of results were later
proved about generalization performance . The key
insight is that generalization performance is related to the
margin of the examples, and that AdaBoost achieves large
Recall that there are over 180,000 rectangle features as-
sociated with each image sub-window, a number far larger
than the number of pixels. Even though each feature can
be computed very efﬁciently, computing the complete set is
prohibitivelyexpensive. Our hypothesis, which is borne out
by experiment, is that a very small number of these features
can be combined to form an effective classiﬁer. The main
challenge is to ﬁnd these features.
In support of this goal, the weak learning algorithm is
designed to select the single rectangle feature which best
separates the positive and negative examples (this is similar
to the approach of  in the domain of image database re-
trieval). For each feature, the weak learner determines the
optimal threshold classiﬁcation function, such that the min-
imum number of examples are misclassiﬁed. A weak clas-
siﬁer thus consists of a feature , a threshold and
a parity indicating the direction of the inequality sign:
Here is a 24x24 pixel sub-window of an image. See Ta-
ble 1 for a summary of the boosting process.
In practice no single feature can perform the classiﬁca-
tion task with low error. Features which are selected in early
rounds of the boosting process had error rates between 0.1
and 0.3. Features selected in later rounds, as the task be-
comes more difﬁcult, yield error rates between 0.4 and 0.5.
3.1. Learning Discussion
Many general feature selection procedures have been pro-
posed (see chapter 8 of  for a review). Our ﬁnal appli-
cation demanded a very aggressive approach which would
discard the vast majority of features. For a similar recogni-
tionproblem Papageorgiouetal. proposed a scheme forfea-
ture selection based on feature variance . They demon-
strated good results selecting 37 features out of a total 1734
Roth et al. propose a feature selection process based
on the Winnow exponential perceptron learning rule .
The Winnow learning process converges to a solution where
many of these weights are zero. Nevertheless a very large
Given example images where
for negative and positive examples respec-
Initialize weights for respec-
and are the number of negatives and
1. Normalize the weights,
so that is a probability distribution.
2. For each feature, , train a classiﬁer which
is restricted to using a single feature. The
error is evaluated with respect to ,
3. Choose the classiﬁer, , withthe lowest error .
4. Update the weights:
where if example is classiﬁed cor-
rectly, otherwise, and .
The ﬁnal strong classiﬁer is:
Table 1: The AdaBoost algorithm for classiﬁer learn-
ing. Each round of boosting selects one feature from the
180,000 potential features.
number of features are retained (perhaps a few hundred or
3.2. Learning Results
While details on the training and performance of the ﬁnal
system are presented in Section 5, several simple results
merit discussion. Initial experiments demonstrated that a
frontal face classiﬁer constructed from 200 features yields
a detection rate of 95% with a false positive rate of 1 in
14084. These results are compelling, but not sufﬁcient for
many real-world tasks. In terms of computation, this clas-
siﬁer is probably faster than any other published system,
requiring 0.7 seconds to scan an 384 by 288 pixel image.
Unfortunately, the most straightforward technique for im-
proving detection performance, adding features to the clas-
siﬁer, directly increases computation time.
For the task of face detection, the initial rectangle fea-
tures selected by AdaBoost are meaningful and easily inter-
preted. The ﬁrst feature selected seems to focus onthe prop-
ertythatthe region of the eyesis oftendarkerthantheregion
Figure 3: The ﬁrst and second features selected by Ad-
aBoost. The two features are shown in the top row and then
overlayed on a typical training face in the bottom row. The
ﬁrst feature measures the difference in intensitybetween the
region of the eyes and a region across the upper cheeks. The
feature capitalizes on the observation that the eye region is
often darker than the cheeks. The second feature compares
the intensities in the eye regions to the intensity across the
bridge of the nose.
of the nose and cheeks (see Figure 3). This feature is rel-
atively large in comparison with the detection sub-window,
and should be somewhat insensitive to size and location of
the face. The second feature selected relies on the property
that the eyes are darker than the bridge of the nose.
4. The Attentional Cascade
This section describes an algorithm for constructing a cas-
cade of classiﬁers which achieves increased detection per-
formance while radically reducing computation time. The
key insight is that smaller, and therefore more efﬁcient,
boosted classiﬁers can be constructed which reject many of
the negative sub-windows while detecting almost all posi-
tive instances (i.e. the threshold of a boosted classiﬁer can
be adjusted so that the false negative rate is close to zero).
Simpler classiﬁers are used to reject the majority of sub-
windows before more complex classiﬁers are called upon
to achieve low false positive rates.
The overall form of the detection process is that of a de-
generate decision tree, what we call a “cascade” (see Fig-
ure 4). A positive result from the ﬁrst classiﬁer triggers the
evaluation of a second classiﬁer which has also been ad-
justed to achieve very high detectionrates. A positive result
from the second classiﬁer triggers a third classiﬁer, and so
on. A negative outcome at any point leads to the immediate
rejection of the sub-window.
Stages in the cascade are constructed by training clas-
siﬁers using AdaBoost and then adjusting the threshold to
minimize false negatives. Note that the default AdaBoost
threshold is designed to yield a low error rate on the train-
ing data. In general a lower threshold yields higher detec-
1 2 3
Figure 4: Schematic depiction of a the detection cascade.
A series of classiﬁers are applied to every sub-window. The
initial classiﬁer eliminates a largenumber of negative exam-
ples with verylittle processing. Subsequent layers eliminate
additionalnegativesbutrequire additionalcomputation. Af-
ter several stages of processing the number of sub-windows
have been reduced radically. Further processing can take
any form such as additional stages of the cascade (as in our
detection system) or an alternative detection system.
tion rates and higher false positive rates.
For example an excellent ﬁrst stage classiﬁer can be con-
structed from a two-feature strong classiﬁer by reducing the
threshold to minimize false negatives. Measured against a
validation training set, the threshold can be adjusted to de-
tect 100% of the faces with a false positive rate of 40%. See
Figure 3 for a description of the two features used in this
Computation of the two feature classiﬁer amounts to
about 60 microprocessor instructions. It seems hard to
imagine that any simpler ﬁlter could achieve higher rejec-
tion rates. By comparison, scanning a simple image tem-
plate, or a single layer perceptron, would require at least 20
times as many operations per sub-window.
The structure of the cascade reﬂects the fact that
within any single image an overwhelming majority of sub-
windows are negative. As such, the cascade attempts to re-
ject as many negatives as possible at the earliest stage pos-
sible. While a positive instance will trigger the evaluation
of every classiﬁer in the cascade, this is an exceedingly rare
Much like a decision tree, subsequent classiﬁers are
trained using those examples which pass through all the
previous stages. As a result, the second classiﬁer faces a
more difﬁcult task than the ﬁrst. The examples which make
it through the ﬁrst stage are “harder” than typical exam-
ples. The more difﬁcult examples faced by deeper classi-
ﬁers push the entire receiver operating characteristic (ROC)
curve downward. At a given detection rate, deeper classi-
ﬁers have correspondingly higher false positive rates.
4.1. Training a Cascade of Classiﬁers
The cascade training process involves two types of trade-
offs. In most cases classiﬁers with more features will
achieve higher detection rates and lower false positive rates.
At the same time classiﬁers with more features require more
time to compute. In principle one could deﬁne an optimiza-
tion framework in which: i) the number of classiﬁer stages,
ii) the number of features in each stage, and iii) the thresh-
old of each stage, are traded off in order to minimize the
expected number of evaluated features. Unfortunately ﬁnd-
ing this optimum is a tremendously difﬁcult problem.
In practice a very simple framework is used to produce
an effective classiﬁer which is highly efﬁcient. Each stage
in the cascade reduces the false positive rate and decreases
the detection rate. A target is selected for the minimum
reduction in false positives and the maximum decrease in
detection. Each stage is trained by adding features until the
target detection and false positivesrates are met ( these rates
are determined by testing the detector on a validation set).
Stages are added until the overall target for false positive
and detection rate is met.
4.2. Detector Cascade Discussion
Thecomplete face detection cascadehas 38 stages with over
6000 features. Nevertheless the cascade structure results in
fast average detection times. On a difﬁcult dataset, con-
taining 507 faces and 75 million sub-windows, faces are
detected using an average of 10 feature evaluations per sub-
window. In comparison, this system is about 15 times faster
than an implementation of the detection system constructed
by Rowley et al.
A notion similar to the cascade appears in the face de-
tection system described by Rowley et al. in which two de-
tection networks are used . Rowley et al. used a faster
yet less accurate network to prescreen the image in order to
ﬁnd candidate regions for a slower more accurate network.
Though it is difﬁcult to determine exactly, it appears that
Rowley et al.’s two network face system is the fastest exist-
ing face detector.
The structure of the cascaded detection process is es-
sentially that of a degenerate decision tree, and as such is
related to the work of Amit and Geman . Unlike tech-
niques which use a ﬁxed detector, Amit and Geman propose
an alternative point of view where unusual co-occurrences
of simple image features are used to trigger the evaluation
of a more complex detection process. In this way the full
detection process need not be evaluated at many of the po-
tential image locations and scales. While this basic insight
Henry Rowley very graciously supplied us with implementations of
his detection system for direct comparison. Reported results are against
his fastest system. It is difﬁcult to determine from the published literature,
but the Rowley-Baluja-Kanade detector is widely considered the fastest
detection system and has been heavily tested on real-world problems.
Other published detectors have either neglected to discuss perfor-
mance in detail, or have never published detection and false positive rates
on a large and difﬁcult training set.
is very valuable, in their implementation it is necessary to
ﬁrst evaluate some feature detector at every location. These
featuresare thengrouped to ﬁnd unusual co-occurrences. In
practice, since the form of our detector and the features that
it uses are extremely efﬁcient, the amortized cost of evalu-
ating our detector at every scale and location is much faster
than ﬁnding and grouping edges throughout the image.
In recent work Fleuret and Geman have presented a face
detection technique which relies on a “chain” of tests in or-
der to signify the presence of a face at a particular scale and
location . The image properties measured by Fleuret and
Geman, disjunctions of ﬁne scale edges, are quite different
than rectangle features which are simple, exist at all scales,
and are somewhat interpretable. The two approaches also
differ radically in their learning philosophy. The motivation
for Fleuret and Geman’s learning process is density estima-
tion and density discrimination, while our detector is purely
discriminative. Finally the false positive rate of Fleuret and
Geman’s approach appears to be higher than that of previ-
ous approaches like Rowley et al. and this approach. Un-
fortunately the paper does not report quantitative results of
this kind. The included example images each have between
2 and 10 false positives.
A 38 layer cascaded classiﬁer was trained to detect frontal
upright faces. To train the detector, a set of face and non-
face training images were used. The face training set con-
sisted of 4916 hand labeled faces scaled and aligned to a
base resolution of 24 by 24 pixels. The faces were ex-
tracted from images downloaded during a random crawl of
the world wide web. Some typical face examples are shown
in Figure 5. The non-face subwindows used to train the
detector come from 9544 images which were manually in-
spected and found to not contain any faces. There are about
350 million subwindows within these non-face images.
The number of features in the ﬁrst ﬁve layers of the de-
tector is 1, 10, 25, 25 and 50 features respectively. The
remaining layers have increasingly more features. The total
number of features in all layers is 6061.
Each classiﬁer in the cascade was trained with the 4916
training faces (plus their vertical mirror images for a total
of 9832 training faces) and 10,000 non-face sub-windows
(also of size 24 by 24 pixels) using the Adaboost training
procedure. For the initial one feature classiﬁer, the non-
face training examples were collected by selecting random
sub-windows from a set of 9544 images which did not con-
tain faces. The non-face examples used to train subsequent
layers were obtained by scanning the partial cascade across
the non-face images and collecting false positives. A max-
imum of 10000 such non-face sub-windows were collected
for each layer.
Speed of the Final Detector
Figure 5: Example of frontal upright face images used for
The speed of the cascaded detector is directly related to
the number of features evaluated per scanned sub-window.
Evaluated on the MIT+CMU test set , an average of 10
featuresout of a total of 6061 are evaluated per sub-window.
This is possible because a large majority of sub-windows
are rejected by the ﬁrst or second layer in the cascade. On
a 700 Mhz Pentium III processor, the face detector can pro-
cess a 384 by 288 pixel image in about .067 seconds (us-
ing a starting scale of 1.25 and a step size of 1.5 described
below). This is roughly 15 times faster than the Rowley-
Baluja-Kanadedetector and about 600 times faster than
the Schneiderman-Kanade detector .
All example sub-windows used for training were vari-
ance normalized to minimize the effect of different light-
ing conditions. Normalization is therefore necessary during
detection as well. The variance of an image sub-window
can be computed quickly using a pair of integral images.
Recall that , where is the standard
deviation, is the mean, and is the pixel value within
the sub-window. The mean of a sub-window can be com-
puted using the integral image. The sum of squared pixels
is computed using an integral image of the image squared
(i.e. two integral images are used in the scanning process).
During scanning the effect of image normalization can be
achieved by post-multiplying the feature values rather than
pre-multiplying the pixels.
Scanning the Detector
The ﬁnal detector is scanned across the image at multi-
ple scales and locations. Scaling is achieved by scaling the
detector itself, rather than scaling the image. This process
makes sense because the features can be evaluated at any
10 31 50 65 78 95 167
Viola-Jones 76.1% 88.4% 91.4% 92.0% 92.1% 92.9% 93.9%
Viola-Jones (voting) 81.1% 89.7% 92.1% 93.1% 93.1% 93.2 % 93.7%
Rowley-Baluja-Kanade 83.2% 86.0% - - - 89.2% 90.1%
Schneiderman-Kanade - - - 94.4% - - -
Roth-Yang-Ahuja - - - - (94.8%) - -
Table 2: Detection rates for various numbers of false positives on the MIT+CMU test set containing 130 images and 507
scale with the same cost. Good results were obtained using
a set of scales a factor of 1.25 apart.
The detector is also scanned across location. Subsequent
locations are obtained byshifting the window some number
of pixels . This shifting process is affected by the scale of
the detector: if the current scale is the window is shifted
by , where is the rounding operation.
The choice of affects both the speed of the detector as
well as accuracy. The results we present are for .
We can achieve a signiﬁcant speedup by setting
with only a slight decrease in accuracy.
Integration of Multiple Detections
Since the ﬁnal detector is insensitive to small changes in
translation and scale, multiple detections will usually occur
aroundeach face in a scanned image. The same is often true
of some types of false positives. In practice it often makes
sense to return one ﬁnal detection per face. Toward this end
it is useful to postprocess the detected sub-windows in order
to combine overlapping detections into a single detection.
In these experiments detections are combined in a very
simple fashion. The set of detections are ﬁrst partitioned
into disjoint subsets. Two detections are in the same subset
if their bounding regions overlap. Each partition yields a
single ﬁnal detection. The corners of the ﬁnal bounding
region are the average of the corners of all detections in the
Experiments on a Real-World Test Set
We tested our system on the MIT+CMU frontal face test
set . This set consists of 130 images with 507 labeled
frontal faces. A ROC curve showingthe performance of our
detector on this test set is shown in Figure 6. To create the
ROC curve the threshold of the ﬁnal layer classiﬁer is ad-
justed from to . Adjusting the threshold to
will yield a detection rate of 0.0 and a false positive rate
of 0.0. Adjusting the threshold to , however, increases
both the detection rate and false positive rate, but only to a
certain point. Neither rate can be higher than the rate of the
detection cascade minus the ﬁnal layer. In effect, a thresh-
old of is equivalent to removing that layer. Further
increasing the detection and false positive rates requires de-
creasing the threshold of the next classiﬁer in the cascade.
Thus, in order to construct a complete ROC curve, classiﬁer
layers are removed. We use the number of false positives as
opposed to the rate of false positives for the x-axis of the
ROC curve to facilitate comparison with other systems. To
compute the false positive rate, simply divide by the total
number of sub-windows scanned. In our experiments, the
number of sub-windows scanned is 75,081,800.
Unfortunately, most previous published results on face
detection have only included a single operating regime (i.e.
single point on the ROC curve). To make comparison with
our detector easier we have listed our detection rate for the
false positive rates reported by the other systems. Table 2
lists the detection rate for various numbers of false detec-
tions for our system as well as other published systems. For
the Rowley-Baluja-Kanade results , a number of differ-
ent versions of their detector were tested yielding a number
of different results they are all listed in under the same head-
ing. For the Roth-Yang-Ahuja detector , they reported
their result on the MIT+CMU test set minus 5 images con-
taining line drawn faces removed.
Figure 7 shows the output of our face detector on some
test images from the MIT+CMU test set.
A simple voting scheme to further improve results
In table 2 we also show results from running three de-
tectors (the 38 layer one described above plus two similarly
trained detectors) and outputting the majority vote of the
three detectors. This improves the detection rate as well as
eliminating more false positives. The improvement would
be greater if the detectors were more independent. The cor-
relation of their errors results in a modest improvementover
the best single detector.
We have presented an approach for object detection which
minimizes computationtime while achieving high detection
accuracy. The approach was used to construct a face de-
tection system which is approximately 15 faster than any
This paper brings together new algorithms, representa-
tions, and insights which are quite generic and may well
Figure 7: Output of our face detector on a number of test images from the MIT+CMU test set.
Figure 6: ROC curve for our face detector on the
MIT+CMU test set. The detector was run using a step size
of 1.0 and starting scale of 1.0 (75,081,800 sub-windows
have broader application in computer vision and image pro-
Finally this paper presents a set of detailed experiments
on a difﬁcult face detection dataset which has been widely
studied. This dataset includes faces under a very wide range
of conditions including: illumination, scale, pose, and cam-
era variation. Experiments on such a large and complex
dataset are difﬁcult and time consuming. Nevertheless sys-
tems which work under these conditions are unlikely to be
brittle or limited to a single set of conditions. More impor-
tantly conclusions drawn from this dataset are unlikely to
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