L EARNING WITH FEATURE - DEPENDENT LABEL NOISE : A PROGRESSIVE APPROACH
A BSTRACT
Label noise is frequently observed in real-world large-scale datasets.
The noise is introduced due to a variety of reasons; it is heterogeneous and feature-dependent.
Most existing approaches to handling noisy labels fall into two categories: they either assume an ideal feature-independent noise, or remain heuristic without theoretical guarantees.
In this paper, we propose to target a new family of featuredependent label noise, which is much more general than commonly used i.i.d.
label noise and encompasses a broad spectrum of noise patterns.
Focusing on this general noise family, we propose a progressive label correction algorithm that iteratively corrects labels and reﬁnes the model.
We provide theoretical guarantees showing that for a wide variety of (unknown) noise patterns, a classiﬁer trained with this strategy converges to be consistent with the Bayes classiﬁer.
In experiments, our method outperforms SOTA baselines and is robust to various noise types and levels.
I NTRODUCTION
Addressing noise in training set labels is an important problem in supervised learning.
Incorrect annotation of data is inevitable in large-scale data collection, due to intrinsic ambiguity of data/class and mistakes of human/automatic annotators (Yan et al., 2014; Andreas et al., 2017).
Developing methods that are resilient to label noise is therefore crucial in real-life applications.
Classical approaches take a rather simplistic i.i.d.
assumption on the label noise, i.e., the label corruption is independent and identically distributed and thus is feature-independent.
Methods based on this assumption either explicitly estimate the noise pattern (Reed et al., 2014; Patrini et al., 2017;
Dan et al., 2019; Xu et al., 2019) or introduce extra regularizer/loss terms (Natarajan et al., 2013;
Van Rooyen et al., 2015; Xiao et al., 2015; Zhang & Sabuncu, 2018; Ma et al., 2018; Arazo et al., 2019; Shen & Sanghavi, 2019).
Some results prove that the commonly used losses are naturally robust against such i.i.d.
label noise (Manwani & Sastry, 2013; Ghosh et al., 2015; Gao et al., 2016;
Ghosh et al., 2017; Charoenphakdee et al., 2019; Hu et al., 2020).
Although these methods come with theoretical guarantees, they usually do not perform as well as expected in practice due to the unrealistic i.i.d.
assumption on noise.
This is likely because label noise is heterogeneous and feature-dependent.
A cat with an intrinsically ambiguous appearance is more likely to be mislabeled as a dog.
An image with poor lighting or severe occlusion can be mislabeled, as important visual clues are imperceptible.
Methods that can combat label noise of a much more general form are very much needed to address real-world challenges.
To adapt to the heterogeneous label noise, state-of-the-arts (SOTAs) often resort to a data-recalibrating strategy.
They progressively identify trustworthy data or correct data labels, and then train using these data (Tanaka et al., 2018;
Wang et al., 2018; Lu et al., 2018; Li et al., 2019).
The models gradually improve as more clean data are collected or more labels are corrected, eventually converging to models of high accuracy.
These data-recalibrating methods best leverage the learning power of deep neural nets and achieve superior performance in practice.
However, their underlying mechanism remains a mystery.
No methods in this category can provide theoretical insights as to why the model can converge to an ideal one.
Thus, these methods require careful hyperparameter tuning and are hard to generalize.
In this paper, we propose a novel and principled method that speciﬁcally targets the heterogeneous, feature-dependent label noise.
Unlike previous methods, we target a much more general family of noise, called Polynomial Margin Diminishing (PMD) label noise.
In this noise family, we allow arbitrary noise level except for data far away from the true decision boundary.
This is consistent with the real-world scenario; data near the decision boundary are harder to distinguish and more likely to be mislabeled.
Meanwhile, a datum far away from the decision boundary is a typical example of its true class and should have a reasonably bounded noise level.
Assuming this new PMD noise family, we propose a theoretically-guaranteed data-recalibrating algorithm that gradually corrects labels based on the noisy classiﬁer’s conﬁdence.
We start from data points with high conﬁdence, and correct the labels of these data using the predictions of the noisy classiﬁer.
Next, the model is improved using cleaned labels.
We continue alternating the label correction and model improvement until it converges.
See Figure 1 for an illustration.
Our main theorem shows that with a theory-informed criterion for label correction at each iteration, the improvement of the label purity is guaranteed.
Thus the model is guaranteed to improve with sufﬁcient rate through iterations and eventually becomes consistent with the Bayes optimal classiﬁer.
Beside the theoretical strength, we also demonstrate the power of our method in practice.
Our method outperforms others on CIFAR-10/100 with various synthetic noise patterns.
We also evaluate our method against SOTAs on three real-world datasets with unknown noise patterns.
To the best of our knowledge, our method is the ﬁrst data-recalibrating method that is theoretically guaranteed to converge to an ideal model.
The PMD noise family encompasses a broad spectrum of heterogeneous and feature-dependent noise, and better approximates the real-world scenario.
It also provides a novel theoretical setting for the study of label noise.
Related works.
We review works that do not assume an i.i.d. label noise.
Menon et al.
(2018) generalized the work of (Ghosh et al., 2015) and provided an elegant theoretical framework, showing that loss functions fulﬁlling certain conditions naturally resist instance-dependent noise.
The method can achieve even better theoretical properties (i e., Bayes-consistency) with stronger assumption on the clean posterior probability η .
In practice, this method has not been extended to deep neural networks.
Cheng et al.
(2020) proposed an active learning method for instance-dependent label noise.
[Figure]
The algorithm iteratively queries clean labels from an oracle on carefully selected data.
However, this approach is not applicable to settings where kosher annotations are unavailable.
Another contemporary work (Chen et al., 2021) showed that the noise in real-world dataset is unlikely to be i.i.d., and proposed to ﬁx the noisy labels by averaging the network predictions on each instance over the whole training process.
While being effective, their method lacks theoretical guarantees.
Chen et al.
(2019) showed by regulating the topology of a classiﬁer’s decision boundary, one can improve the model’s robustness against label noise.
Data-recalibrating methods use noisy networks’ predictions to iteratively select/correct data and improve the models.
Tanaka et al.
(2018) introduced a joint training framework which simultaneously enforces the network to be consistent with its own predictions and corrects the noisy labels during training.
Wang et al.
identiﬁed noisy labels as outliers based on their label consistencies with surrounding data.
Lu et al.
(2018) used a curriculum learning strategy where the teacher net is trained on a small kosher dataset to determine if a datum is clean; then the learnt curriculum that gives the weight to each datum is fed into the student net for the training and inference.
(Yu et al., 2019; Bo et al., 2018) trained two synchronized networks; the conﬁdence and consistency of the two networks are utilized to identify clean data.
Wu et al.
(2020) selected the clean data by investigating the topological structures of the training data in the learned feature space.
For completeness, we also refer to other methods of similar design (Li et al., 2017; Vahdat, 2017;
Andreas et al., 2017; Ma et al., 2018; Thulasidasan et al., 2019; Arazo et al., 2019; Shu et al., 2019; Yi & Wu, 2019).
As for theoretical guarantees, Ren et al.
(2018) proposed an algorithm that iteratively re-weights each data point by solving an optimization problem.
They proved the convergence of the training, but provided no guarantees that the model converges to an ideal one.
Amid et al.
(2019b) generalized the work of (Amid et al., 2019a) and proposed a tempered matching loss.
They showed that when the ﬁnal softmax layer is replaced by the bi-tempered loss, the resulting classiﬁer will be Bayes consistent.
Zheng et al.
(2020) proved a one-shot guarantee for their data-recalibrating method; but the convergence of the model is not guaranteed.
Our method is the ﬁrst data-recalibrating method which is guaranteed to converge to a well-behaved classiﬁer.
M ETHOD
We start by introducing the family of Poly-Margin Diminishing (PMD) label noise.
In Section 2.2, we present our main algorithm.
Finally, we prove the correctness of our algorithm in Section 3.
Notations and preliminaries.
Although the noise setting and algorithm naturally generalize to multiclass, for simplicity we focus on binary classiﬁcation.
Let the feature space be X .
We assume the data ( x , y ) is sampled from an underlying distribution D on X × { 0 , 1 } .
Deﬁne the posterior probability η ( x ) =
P [ y = 1 | x ] .
Let τ 0 , 1 ( x ) =
P [ (cid:101) y
= 1 | y = 0 , x ] and τ 1 , 0 ( x ) =
P [ (cid:101) y
=
| y
= 1 , x ] be the noise functions, where (cid:101)
y denotes the corrupted label.
For example, if a datum x has true label y = 0 , it has τ 0 , 1 ( x ) chance to be corrupted to 1.
Similarly, it has τ 1 , 0 ( x ) chance to be corrupted from 1 to 0.
Let (cid:101) η
( x ) = P [ (cid:101) y
= 1 | x ] be the noisy posterior probability of (cid:101) y
= 1 given feature x .
Let η ∗ ( x ) =
I { η ( x ) ≥ 12 } be the (clean) Bayes optimal classiﬁer, where I A equals 1 if A is true, andotherwise.
Finally, let f ( x ) :
X → [0 , 1] be the classiﬁer scoring function (the softmax output of a neural network in this paper).
2. P OLY -M ARGIN D IMINISHING N OISE
We ﬁrst introduce the family of noise functions τ this paper will address.
We introduce the concept of polynomial margin diminishing noise (PMD noise), which only upper bounds the noise τ in a certain level set of η ( x ) , thus allowing τ to be arbitrarily high outside the restricted domain.
This formulation not only covers the feature-independent scenario but also generalizes scenarios proposed by (Du & Cai, 2015; Menon et al., 2018; Cheng et al., 2020).
Deﬁnition 1 (PMD noise) .
A pair of noise functions τ 0 , 1 ( x ) and τ 1 , 0 ( x ) are polynomial-margin diminishing (PMD), if there exist constants t 0 ∈ (0 , 12 ) , and c 1 , c 2 > 0 such that:
[Equation]
We abuse notation by referring to t 0 as the “margin” of τ .
Note that the PMD condition only requires the upper bound on τ to be polynomial and monotonically decreasing in the region where the Bayes classiﬁer is fairly conﬁdent.
For the region { x : | η ( x ) − 12 | < t 0 } , we allow both τ 0 , 1 ( x ) and τ 1 , 0 ( x ) to be arbitrary.
Figure 2(d) illustrates the upper bound (orange curve) and a sample noise function (blue curve).
We also show the corrupted data according to this noise function (black points are the clean data whereas red points are the data with corrupted labels).
The PMD noise family is much more general than existing noise assumptions.
For example, the boundary consistent noise (BCN) (Du & Cai, 2015; Menon et al., 2018) assumes a noise function that monotonically decreases as the data are moving away from the decision boundary.
See Figure 2(c) for an illustration.
This noise is much more restrictive compared to our PMD noise which (1) only requires a monotonic upper bound, and (2) allows arbitrary noise strength in a wide buffer near the decision boundary.
Figure 2(b) shows a traditional feature-independent noise pattern (Reed et al., 2014;
Patrini et al., 2017), which assumes τ 0 , 1 ( x ) (resp.
τ 1 , 0 ( x ) ) to be a constant independent of x .
[Figure]
2. T HE P ROGRESSIVE C ORRECTION A LGORITHM
Our algorithm iteratively trains a neural network and corrects labels.
We start with a warm-up period, in which we train the neural network (NN) with the original noisy data.
This allows us to attain a reasonable network before it starts ﬁtting noise (Zhang et al., 2017).
After the warm-up period, the classiﬁer can be used for label correction.
We only correct a label on which the classiﬁer f has a very high conﬁdence.
The intuition is that under the noise assumption, there exists a “pure region” in which the prediction of the noisy classiﬁer f is highly conﬁdent and is consistent with the clean
Bayes optimal classiﬁer η ∗ .
Thus the label correction gives clean labels within this pure region.
In particular, we select a high threshold θ .
If f predicts a different label than ˜ y and its conﬁdence is above the threshold, | f ( x ) − 1 / 2 | > θ , we ﬂip the label ˜
y to the prediction of f .
We repeatedly correct labels and improve the network until no label is corrected.
Next, we slightly decrease the threshold θ , use the decreased threshold for label correction, and improve the model accordingly.
We continue the process until convergence.
For convenience in theoretical analysis, in the algorithm, we deﬁne a continuous increasing threshold T and let θ = 1 / 2 − T .
Our algorithm is summarized in
Algorithm 1.
We term our algorithm as PLC (Progressive Label Correction).
In Section 3, we will show that this iterative algorithm will converge to be consistent with clean Bayes optimal classiﬁer η ∗ ( x ) for most of the input instances.
Input: Dataset ˜ S
= { ( x 1 , (cid:101) y 01 ) , · · · , ( x n , (cid:101) y 0 n ) } , initial NN f ( x ) , step size β , initial and end thresholds ( T 0 , T end ) , warm-up m , total round N
Output: f final ( · ) 1: T ← T2: θ ← 1 / 2 − T3: for t ← 1 , · · · , N do 4:
Train f ( x ) on ˜ S 5: for all ( x i , (cid:101)
y t − 1 i ) ∈ ˜ S and | f
( x i ) − 12 | ≥ θ do 6: (cid:101)
y ti ← I { f ( x i ) ≥ 12 } 7: end for 8: if t ≥ m then 9: θ ← 1 / 2 − T 10: if ∀ i ∈ [1 , · · · , n ] , (cid:101)
y ti =
(cid:101)
y t − 1 i then 11:
T ← min( T (1 + β ) , T end ) 12: end if 13: end if 14: ˜ S ← { ( x 1 , (cid:101)
y t 1 ) , · · · , ( x n , (cid:101) y tn ) } 15: end for
Generalizing to the multi-class scenario.
In multi-class scenario, denote by f i ( x ) the classiﬁer’s prediction probability of label i .
Let h x be the classiﬁer’s class prediction, i.e., h x = arg max
i f i ( x ) .
We change the (cid:12)(cid:12) f
( x ) − 12 (cid:12)(cid:12) term to the gap between the highest conﬁdence f h x ( x ) and the conﬁdence on (cid:101)
y , f (cid:101) y
( x ) .
If the absolute difference between these two conﬁdences is larger than certain threshold θ , then we correct (cid:101) y to h x .
In practice, we ﬁnd using the difference of logarithms will be more robust.
A NALYSIS
Our analysis focuses on the asymptotic case and answers the following question: Given inﬁnitely many data with corrupted labels, is it possible to learn a reasonably good classiﬁer?
We show that if the noise satisﬁes the arguably-general PMD condition, the answer is yes.
Assuming mild conditions on the hypothesis class of the machine learning model and the distribution D , we prove that Algorithm 1 obtains a nearly clean classiﬁer.
This reduces the challenge of noisy label learning from a realizable problem into a sample complexity problem.
In this work we only focus on the asymptotic case, and leave the sample complexity for future work.
3. A SSUMPTIONS
Our ﬁrst assumption restricts the model to be able to at least approximate the true Bayes classiﬁer η ( x ) .
This condition assumes that given a hypothesis class H with sufﬁcient complexity, the approximation gap between a classiﬁer f ( x ) in this class and η ( x ) is determined by the inconsistency between the noisy labels and the Bayes optimal classiﬁer.
Deﬁnition 2 (Level set ( α, (cid:15) ) -consistency) .
Suppose data are sampled as ( x , ˜ y ) ∼ D ( x , ˜ η ( x )) and f ( x ) =
arg min h ∈H E ( x , ˜ y )
∼ D ( x , ˜ η
( x )) Loss ( h ( x ) , ˜ y ) .
Given ε < 12 , we call H is ( α, (cid:15) )
-consistent
if:
[Equation]
[Table]
[Equation]
For two input instances z and x such that η ( z ) > η ( x ) (and hence the clean Bayes optimal classiﬁer η ∗ ( x ) has higher conﬁdence at z than it does at x ), the indicator function{ ˜
y
z (cid:54) =
η ∗ ( z ) } (cid:0) z : (cid:12)(cid:12) η
( z ) − 12 (cid:12)(cid:12) ≥ (cid:12)(cid:12)
η
( x ) − 12 (cid:12)(cid:12)(cid:1) equals to 1 if the label of the more conﬁdent point z is inconsistent with η ∗ ( x ) .
This condition says that the approximation error of the classiﬁer at x should be controlled by the risk of η ∗ ( · ) at points z where η ∗ ( · ) is more conﬁdent than it is at x .
We next deﬁne a regularity condition of data distribution which describes the continuity of the level set density function.
Deﬁnition 3 (Level set bounded distribution) .
Deﬁne the margin t ( x ) = | η ( x ) − 12 | and G ( t ) be the cdf of t : G ( t ) =
P x ∼ D ( | η ( x ) − 12 | ≤ t ) .
Let g ( t ) =
G (cid:48) ( t ) be the density function of t .
We say the distribution D is ( c ∗ , c ∗ ) -bounded if for all 0 ≤ t ≤ 1 / 2 , 0 < c ∗ ≤ g ( t ) ≤ c ∗ .
If D is ( c ∗ , c ∗ ) -bounded, we deﬁne the worst-case density-imbalance ratio of D by (cid:96) D :=
c ∗ c ∗ .
The above condition enforces the continuity of level set density function.
This is crucial in the analysis since such a continuity allows one to borrow information from its neighborhood region so that a clean neighbor can help correct the corrupted label.
To simplify the notation, we will omit D in the subscript when we mention (cid:96) .
From now on, we will assume:
Assumption 1.
There exist constants α, (cid:15), c ∗ , c
∗ such that the hypothesis class H is ( α, (cid:15) )
-consistent and the unknown distribution D is ( c ∗ , c ∗ ) -bounded.
3. M AIN R ESULT AND P ROOF S KETCH
In this section we ﬁrst state our main result, and then present the supporting claims.
Complete proofs can be found in the appendix.
Our main result below states that if our starting function is trained correctly, i.e., f ( x ) = arg min h ∈H E ( x , ˜ y ) ∼ D ( x , ˜ η
( x )) Loss ( h ( x ) , ˜ y ) , then Algorithm 1 terminates with most of the ﬁnal labels matching the Bayes optimal classiﬁer labels.
In practice, minimizing true risk is not achievable.
Instead, the empirical risk is used to estimate true risk, approaching true risk asymptotically.
For a scoring function f , we will denote by y f ( x ) :
= I ( f ( x ) ≥ 1 / 2) the label predicted by f .
Theorem 1.
Under Assumption 1, for any noise τ which is PMD with margin t 0 , deﬁne e 0 = max ( t 0 , α + ε 1+2 α ) .
Then for the output of Algorithm 1 with f as above and with the following initializations: (1) T 0 <
12 − e 0 , (2) m ≥ (cid:96)αε log( 2 T 0 1 − 2 e 0 ) , (3) N ≥ m + 1 β log( T 0 3 ε ) , (4) T end ≤ 3 (cid:15) and (5) εα(cid:96) ≤ β ≤ 2 εα(cid:96) , we have:
[Equation]
In the remainder of this section we shall assume that the noise τ is PMD with margin t 0 .
To prove our result we ﬁrst deﬁne a “pure” level set.
Deﬁnition
(Pure ( e, f, η ) -level set) .
A set L ( e, η ) :=
{ x || η ( x ) − 12 | ≥ e } is pure for f if y f ( x ) =
η ∗ ( x ) for all x ∈ L ( e, η ) .
We now state a lemma that forms the foundation of our progressive correction algorithm.
We show that given a tiny region where the model is reliable, we can move one step forward by trusting the model.
Although the improvement is slight in a single round, it empowers a conservatively recursive step in the Algorithm 1.
Lemma 1 (One round purity improvement) .
Suppose Assumption 1 is satisﬁed, and assume an f such that there exists a pure ( e, f, η ) -level set with 3 (cid:15) ≤ e < 12 .
Let ˜ η new ( x ) =
y f ( x ) if | f ( x ) − 1 / 2 | ≥ e and ˜ η
( x ) if | f ( x ) − 1 / 2 | < e , and assume f new = arg min h ∈H E ( x , ˜ y ) ∼ D ( x , ˜
η new ( x ))
Loss ( h ( x ) , ˜ y ) .
Let e new
= min { e | e > 0 , L ( e, η ) is pure for f new } .
Then 12 − e new ≥ (1 + εα(cid:96) )
( 12 − e ) .
The above lemma states that the cleansed region will be enlarged by at least a constant factor.
In the following lemma, we justify the functionality of the ﬁrst m warm-up rounds.
Since the initial neural network can behave badly, the region where we can trust the classiﬁer can be very limited.
Before starting the ﬂipping procedure in a relatively larger level set, one ﬁrst needs to expand the initial tiny region 12 − e 0 to a constant T 0 .
Lemma 2 (Warm-up rounds) .
Suppose for a given function f 0 there exists a level set L ( e 0 , η ) which is pure for f 0 .
Given T 0 < 1 / 2 , after running Algorithm 1 for m ≥ (cid:96)αε log( 2 T 0 1 − 2 e 0 ) rounds, there exists a level set L ( 12 − T 0 , η ) that is pure for f 0 .
Next we present our ﬁnal lemma that combines the previous two lemmata.
Lemma 3.
Suppose Assumption 1 is satisﬁed, and for a given function f 0 there exists a level set
L ( e 0 , η ) which is pure for f 0 .
If one runs Algorithm 1 starting with f 0 and the initializations: (1)
T 0 < 12 − e 0 , (2) m ≥ (cid:96)αε log( 2 T 0 1 − 2 e 0 ) , (3) N ≥ m + 1 β log( 1 − 6 ε 2 T 0 ) , (4) T end ≤ 12 − 3 (cid:15) and (5) ε α(cid:96) ≤ β ≤ 2 ε α(cid:96) , then we have P x ∼ D [ y f final ( x ) =
η ∗ ( x )] ≥ 1 − 3 c ∗ (cid:15) .
This lemma states that given an initial model that has a reasonably pure super level set, one can manage to progressively correct a large fraction of corrupted labels by running Algorithm 1 for a sufﬁcient long time with carefully chosen parameters.
The limit of Algorithm 1 will depend on the approximation ability of the neural network, which is characterized by parameter ε in Deﬁnition 2.
To prove Theorem 1 using Lemma 3, it sufﬁces to get a model which has a reliable region.
This is provably achievable by training with a family of good scoring functions on PMD noisy data.
E XPERIMENTS
We evaluate our method on both synthetic and real-world datasets.
We ﬁrst conduct synthetic experiments on two public datasets CIFAR-10 and CIFAR-100 (Krizhevsky et al., 2009).
To synthesize the label noise, we ﬁrst approximate the true posterior probability η using the conﬁdence prediction of a clean neural network (trained with the original clean labels).
We call these original labels raw labels .
Then we sample y x ∼ η ( x ) for each instance x .
Instead of using raw labels, we use these sampled labels y x
as the clean labels, whose posterior probabilities are exactly η ( x ) ; and therefore the neural network is the Bayes optimal classiﬁer η ∗ : X → { 1 , · · · , C } , where C is the number of classes.
Note that in multi-class setting, η ( x ) has a vector output and η i ( x ) is the i -th element of this vector.
Noise generation.
We consider a generic family of noise.
We consider not only feature-dependent noise, but also hybrid noise that consists of both feature-dependent noise and i.i.d.
noise.
For feature-dependent noise, we use three types of noise functions within the PMD noise family.
To make the noise challenging enough, for input x we always corrupt label from the most conﬁdent category u x to the second conﬁdent category s x , according to η ( x ) .
Because s x is the class that confuses η ∗ ( x ) the most, this noise will hurt the network’s performance the most.
Note that y x is sampled from η ( x ) , which has quite an extreme conﬁdence.
Thus we generally assume y x is u x .
For each datum x , we only ﬂip it to s x or keep it as u x .
The three noise functions are as follows:
Type-I : τ u x ,s x = − 1 2 [ η u x ( x )
− η s x ( x )] 2 + 1 2 , Type-II : τ u x ,s x = 1 − [ η u x ( x ) − η s x ( x )] 3 , Type-III :
τ u x ,s x = 1 − 1 3 (cid:104) [ η u x ( x ) − η s x ( x )] 3 + [ η u x ( x ) − η s x ( x )] 2 + [ η u x ( x ) − η s x ( x )] (cid:105) .
Notice that the noise level is determined by the η ( x ) naturally and we cannot control it directly.
To change the noise level, we multiply τ u x ,s x by a certain constant factor such that the ﬁnal proportion of noise matches our requirement.
For PMD noise only, we test noise levels 35% and 70%, meaning that 35% and 70% of the data are corrupted due to the noise, respectively.
For i.i.d.
noise we follow the convention and adopt the commonly used uniform noise and asymmetric noise (Patrini et al., 2017).
We artiﬁcially corrupt the labels by constructing the noise transition matrix T , where T ij = P ( (cid:101) y =
j | y
= i ) =
τ ij deﬁnes the probability that a true label y
= i is ﬂipped to j .
Then for each sample with label i , we replace its label with the one sampled from the probability distribution given by the i -th row of matrix T .
We consider two kinds of i.i.d.
noise in this work.
(1) Uniform noise: the true label i is corrupted
uniformly to other classes, i.e., T ij = τ/
C
−
) for i
(cid:54)
=
j , and T ii = 1 − τ , where τ is the constant noise level; (2) Asymmetric noise: the true label i is
ﬂipped to j or stays unchanged with probabilities T ij = τ and T ii = 1 − τ , respectively.
Baselines.
We compare our method with several recently proposed approaches.
(1) GCE (Zhang & Sabuncu, 2018); (2) Co-teaching+ (Yu et al., 2019); (3) SL (Wang et al., 2019); (4) LRT (Zheng et al., 2020).
All these methods are generic and handle the label noise without assuming the noise structures.
Finally, we also provide the results by standard method, which simply trains the deep network on noisy datasets in a standard manner.
During training, we use a batch size of 128 and train the network for 180 epochs to ensure the convergence of all methods.
We train the network with SGD optimizer, with initial learning rate 0.01.
We randomly repeat the experiments 3 times, and report the mean and standard deviation values.
Our code is available at https://github.com/pxiangwu/PLC .
Results.
Table 1 lists the performance of different methods under three types of feature-dependent noise at noise levels 35% and 70%.
We observe that our method achieves the best performance across different noise settings.
Moreover, notice that some of the baseline methods’ performances are inferior to the standard approach.
Possible reasons are that these methods behave too conservatively in dealing with noise.
Thus they only make use of a small subset of the original training set, which is not representative enough to grant the model good discriminative ability.
In Table 2 we show the results on datasets corrupted with a combination of feature-dependent noise and i.i.d.
noise, which ends up to real noise levels ranging from 50% to 70% (in terms of the proportion of corrupted labels).
I.i.d. noise is overlayed on the feature-dependent noise.
Our method outperforms baselines under these more complicated noise patterns.
In contrast, when the noise level is high like the cases where we further apply additional 30% and 60% uniform noise, performances of a few baselines deteriorate and become worse than the standard approach.
We carry out the ablation studies on hyper-parameters θ 0 (determining the initial conﬁdence threshold for label correction, see Algorithm 1) and
β (the step size).
In Tables 3 and 4, we show that our method is robust against the choice of θ 0 and β up to a wide range.
Notice that to compare against the threshold θ 0 , here we are calculating the absolute difference of log f (cid:101) y
( x ) and log f h x ( x ) .
As mentioned in Section 2.2, this operation gives a good performance in practice.
[Table]
are reported
[Table]
We use CIFAR-10 with 35% feature-dependent noise, and set β = 0 . 1 .
[Table]
We use CIFAR-10 with 35% feature-dependent noise, and set exp ( θ 0 ) =
[Table] [Table]
Results on real-world noisy datasets.
To test the effectiveness of the proposed method under realworld label noise, we conduct experiments on the Clothing1M dataset (Xiao et al., 2015).
This dataset contains 1 million clothing images obtained from online shopping websites with 14 categories.
The labels in this dataset are quite noisy with an unknown underlying structure.
This dataset provides 50 k ,
14 k and 10 k manually veriﬁed clean data for training, validation and testing, respectively.
Following (Tanaka et al., 2018; Yi & Wu, 2019), in our experiment we discard the 50 k clean training data and evaluate the classiﬁcation accuracy on the 10 k clean data.
Also, following (Yi & Wu, 2019), we use a randomly sampled pseudo-balanced subset as the training set, which includes about 260 k images.
We set the batch size 32, learning rate 0.001, and adopt SGD optimizer and use ResNet-50 with weights pre-trained on ImageNet, as in (Tanaka et al., 2018;
Yi & Wu, 2019).
We compare our method with the following baselines.
(1) Standard; (2) Forward Correction (Patrini et al., 2017); (3) D2L
(Ma et al., 2018); (4) JO (Tanaka et al., 2018); (5) PENCIL (Yi & Wu, 2019); (6)
DY (Arazo et al., 2019); (7) GCE (Zhang & Sabuncu, 2018); (8) SL (Wang et al., 2019); (9) MLNT (Li et al., 2019); (10) LRT (Zheng et al., 2020).
In Table 5 we observe that our method achieves the best performance, suggesting the applicability of our label correction strategy in real-world scenarios.
Apart from Clothing1M, we also test our method on another smaller dataset, Food-101N (Lee et al., 2018).
Food-101N is a dataset for food classiﬁcation, and consists of 310k training images collected from the web.
The estimated label purity is 80%.
Following (Lee et al., 2018), the classiﬁcation accuracy is evaluated on the Food-101 (Bossard et al., 2014) testing set, which contains 25k images with curated annotations.
We use ResNet-50 pre-trained on ImageNet.
We train the network for 30 epochs with SGD optimizer.
The batch size is 32 and the initial learning rate is 0.005, which is divided by 10 every 10 epochs.
We also adopt simple data augmentation procedures, including random horizontal ﬂip, and resizing the image with a short edge of 256 and then randomly cropping a 224x224 patch from the resized image.
We repeat the experiments with 3 random trials and report the mean value and standard deviation.
The results are shown in Table 6.
Our method much improves upon the previous approaches.
Finally, we test our method on a recently proposed real-world dataset, ANIMAL-10N (Song et al., 2019).
This dataset contains human-labeled online images for 10 animals with confusing appearance.
The estimated label noise rate is 8%.
There are 50,000 training and 5,000 testing images.
Following (Song et al., 2019), we use VGG-19 with batch normalization.
The SGD optimizer is employed.
Also following (Song et al., 2019), we train the network for 100 epochs and use an initial learning rate of 0.1, which is divided by 5 at 50% and 75% of the total number of epochs.
We repeat the experiments with 3 random trials and report the mean value and standard deviation.
As is shown in Table 7, our method outperforms the existing baselines.
[Table]
[Table] [Table]
C ONCLUSION
We propose a novel family of feature-dependent label noise that is much more general than the traditional i.i.d.
noise pattern.
Building upon this noise assumption, we propose the ﬁrst datarecalibrating method that is theoretically guaranteed to converge to a well-behaved classiﬁer.
On the synthetic datasets, we show that our method outperforms various baselines under different featuredependent noise patterns subject to our assumption.
Also, we test our method on different real-world noisy datasets and observe superior performances over existing approaches.
The proposed noise family offers a new theoretical setting for the study of label noise.
Acknowledgement.
The authors acknowledge support from US National Science Foundation (NSF) awards CRII-1755791, CCF-1910873, CCF-1855760.
This effort was partially supported by the
Intelligence Advanced Research Projects Agency (IARPA) under the contract W911NF20C0038.
The content of this paper does not necessarily reﬂect the position or the policy of the Government, and no ofﬁcial endorsement should be inferred.
A A PPENDIX
Lemma 1 (One round purity improvement) .
Suppose Assumption 1 is satisﬁed and assume an f such that there exists a pure ( e, f, η ) -level set with 3 (cid:15) ≤ e < 12 .
Let ˜ η new ( x ) =
y f ( x ) if | f ( x ) − 1 / 2 | ≥ e and ˜ η
( x ) if | f ( x ) − 1 / 2 | < e and assume f new = arg min h ∈H E ( x , ˜ y ) ∼ D ( x , ˜
η new ( x ))
Loss ( h ( x ) , ˜ y ) .
Let e new
= min { e | e > 0 , L ( e, η ) is pure for f new } .
Then 12 − e new ≥ (1 + εα(cid:96) )
( 12 − e ) .
Proof : We analyze the case where η ( x ) > 12 .
The analysis on the other side can be derived similarly.
Due to the fact that there exists a level set L ( e, η ) pure to f , we have e ≤ | η ( x ) − 12 | , ∀ x :
[Equation]
(cid:12)(cid:12)(cid:12)(cid:12)
[Equation]
(cid:12)(cid:12)(cid:12)(cid:12)
[Equation] [Equation] − 1 2 (cid:12)(cid:12)(cid:12)(cid:12)(cid:21) = 0 . Now consider x where e − γ ≤ | η ( x ) − 12 | .
Since the distribution D is ( c ∗ , c ∗ ) -bounded, we have:
E ( z , ˜ y ) ∼ ( D, ˜ η new ( z ))
[ 1 { ˜ y z (cid:54) =
η ∗ ( z ) } ( z ) ||
η ( z ) − 1 2 | ≥ | η ( x ) − 1 2 | ]
= P z
[˜ y z (cid:54) =
η ∗ ( z ) ||
η ( z ) − 1 2 | ≥ | η ( x ) − 1 2 | ]
= P z
[˜ y z (cid:54) =
η ∗ ( z ) , | η ( z ) − 12 | ≥ | η ( x ) − 12 | ]
P z [ | η ( z ) − 12 | ≥ | η ( x ) − 12 | ] ≤ P z
[˜ y z (cid:54) =
η ∗ ( z ) , 12 + e − γ ≤ η ( z ) ≤ 12 + e ]
P z [ | η ( z ) − 12 | ≥ | η ( x ) − 12 | ]
+ P z
[˜ y z (cid:54) =
η ∗ ( z ) , 12 − e ≤ η ( z ) ≤ 12 − e + γ ] P
[Equation]
If ε(cid:96)α ( 12 − e ) ≤ γ ≤ 2 ε(cid:96)α ( 12 − e ) , the impurity in super level set 12 + e − γ is at most 2 (cid:15)α .
The level set ( α, ε ) -consistency condition implies | f new ( x ) − η ( x ) | ≤ 3 (cid:15) for x s.t.
e − γ ≤ | η ( x ) − 12 | .
If e ≥ 3 (cid:15) , f new ( x ) will give the same label as η ∗ ( x ) and thus ( e − γ, η ) -level set becomes pure for f .
Meanwhile, the choice of γ ensures that 12 − e new ≥ (1 + ε(cid:96)α )( 12 − e ) .
Lemma 2 (Warm-up rounds) .
Suppose for a given function f 0 there exists a level set L ( e 0 , η ) which is pure for f 0 .
Given T 0 < 1 / 2 , after running Algorithm 1 for m ≥ (cid:96)αε log( 2 T 0 1 − 2 e 0 ) rounds, there exists a level set L ( 1 2 − T 0 , η ) that is pure for f 0 .
Proof : The proof follows from the fact that each round of label ﬂipping improves the purity by a factor of (1 + ε(cid:96)α ) .
To obtain an at least T 0 pure region, it sufﬁces to repeat the ﬂipping step for m ≥ (cid:96)αε log( T 0 1 − 2 e 0 ) rounds.
Lemma 3.
Suppose Assumption 1 is satisﬁed, and for a given function f 0 there exists a level set
L ( e 0 , η ) which is pure for f 0 .
If one runs Algorithm 1 starting with f 0 and the initializations: (1)
T 0 < 12 − e 0 , (2) m ≥ (cid:96)αε log( 2 T 0 1 − 2 e 0 ) , (3) N ≥ m + 1 β log( 1 − 6 ε 2 T 0 ) , (4) T end ≤ 12 − 3 (cid:15) and (5) εα(cid:96) ≤ β ≤ 2 εα(cid:96) , then we have P x ∼ D [ y f final ( x ) =
η ∗ ( x )] ≥ 1 − 3 c ∗ (cid:15) .
Proof : The proof can be done by combining Lemma 1 and Lemma 2.
In the ﬁrst m iterations, by
Lemma 2, we can guarantee a level set ( 12 − T 0 , η ) pure to f .
In the rest of the iterations we ensure the level set | η ( x ) − 12 | ≥ 12 − T is pure.
We increase T by a reasonable factor of β to avoid incurring too many corrupted labels while ensuring enough progress in label puriﬁcation, i.e., εα(cid:96) ≤ β ≤ 2 εα(cid:96) , such that in the level set | η ( x ) − 12 | ≥ 12 − T we have | f ( x ) − η ( x ) | ≤ 3 ε .
This condition ensures the correctness of ﬂipping when T ≤ 12 − 3 ε .
The purity cannot be improved once T ≥ 12 − 3 ε
= T end since there is no guarantee that f ( x ) has consistent label with η ( x ) when | η ( x ) − 12 | < 3 ε and | η ( x ) − f ( x ) | ≤ 3 ε .
By ( c ∗ , c ∗ ) -bounded assumption on D , its mass of impure 3 ε level set region is at most 3 c ∗ (cid:15) .
Theorem 1.
Under assumption 1, for any noise τ which is PMD with margin t 0 , deﬁne e 0 = max ( t 0 , α + ε 1+2 α ) .
Then for the output of Algorithm 1 with f as above and with the following initializations: (1) T 0 <
12 − e 0 , (2) m ≥ (cid:96)αε log( 2 T 0 1 − 2 e 0 ) , (3) N ≥ m + 1 β log( T 0 3 ε ) , (4) T end ≤ 3 (cid:15) and (5) εα(cid:96) ≤ β ≤ 2 εα(cid:96) , we have:
[Equation]
Proof : The proof is based on Lemma 3 plus a veriﬁcation of the existence of f 0 for which there exists a pure ( e 0 , f, η ) -level set.
Let:
[Equation]
In the level set | η ( x ) − 12 | ≥ e 0 , P z
[˜ y z (cid:54) =
η ∗ ( z ) | | η ( z ) − 12 | ≥ e 0 ] ≤ 12 − e
+ τ ( z ) .
By level set ( α, ε ) -consistency, it sufﬁces to satisfy α ( 12 − e o + τ ) + ε ≤ e 0 to ensure that f ( x ) has the same prediction with η ( x ) when | η ( x ) − 12 | ≥ e 0 .
By polynomial level set diminishing noise, we have τ ( x ) ≤ 12 − e 0 if e 0 > t 0 , and thus by choosing e 0 = max ( t 0 , α + ε 1+2 α ) one can ensure that initial fhas a pure ( e 0 , f 0 , η ) -level set.
The rest of the proof follows from Lemma 3.