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Georgian Mathematical Journal 1(1994), No. 2, 197-212

LIMIT DISTRIBUTION OF THE INTEGRATED SQUARED ERROR OF TRIGONOMETRIC SERIES REGRESSION

ESTIMATOR

E. NADARAYA

Abstract. Limit distribution is studied for the integrated squared error of the projection regression estimator (2) constructed on the basis of independent observations (1). By means of the obtained limit theorems, a test is given for verifying the hypothesis on the regression, and the power of this test is calculated in the case of Pitman alternatives.

Let observationsY1, Y2, . . . , Yn be represented as

Yi =µ(xi) +εi, i= 1, n, (1) whereµ(x),x∈[−π, π], is the unknown regression function to be estimated by observations Yi; xi, i= 1, n, are the known numbers, and −π= x0 <

x1 <· · · < xn ≤π, εi, i = 1, n, are independent equidistributed random variables;1= 0,21=σ2, and 41<∞.

The problem of nonparametric estimation of the regression functionµ(x) for the model (1) has a recent history and has been treated only in few papers. In particular, a kernel estimator of the Rosenblatt–Parzen type for µ(x) was proposed for the first time in [1].

Assume that µ(x) is representable as a converging series in L2(−π, π) with respect to the orthonormal trigonometric system

n

(2π)1/2, π1/2cosix, π1/2sinixo

i=1.

Consider the estimator of the functionµ(x) constructed by the projection method of N.N. Chentsov [2]

µnN(x) = a0n

2 + XN i=1

aincosix+binsinix, (2)

1991Mathematics Subject Classification. 62G07.

197

(2)

whereN =N(n)→ ∞forn→ ∞and ain= 1

π Xn j=1

Yjjcosixj, bin= 1 π

Xn j=1

Yjjsinixj,

j =xj−xj1, j= 1, n, i= 0, N .

The estimator (2) can be rewritten in a more compact way as µnN =

Xn j=1

YjjKN(x−xj), whereKN(u) =1 P

|r|≤N

eiru is the Dirichlet kernel.

In [3], p.347, N.V. Smirnov considered estimators of the type (2) for a specially chosen class of functions µ(x) in the case of equidistant points xj[−π, π] and of independent and normally distributed observation errors εi. In [4] an estimator of the type (2) is obtained, which is asymptotically equivalent to projection estimators which are optimal in the sense of some accuracy criterion. The asymptotics of the mean value of the integrated squared error of the estimator (2) is considered in [5].

It is of interest to investigate the limit distribution of the integrated

squared error Z π

π

nN(x)−µ(x)]2dx,

which is the goal pursued in this paper. The method used to prove the theorems below is based on the functional limit theorem for a sequence of semimartingales [6].

Denote

UnN = n 2π(2N+ 1)

Z π

π

‚µnN(x)−EµnN(x)ƒ2

dx,

Qir= ∆irKN(xi−xr), σ2nN = n2σ4 π2(2N+ 1)2

Xn r=2

r1

X

j=1

Q2jr, ηik= n

π(2N+ 1)σnN

εiεkQik,

ξ1= 0, ξk=

k1

X

i=1

ηik, k= 2, n, ξk= 0, k > n,

and assume that Fk is σ-algebra generated by random variables ε1, ε2, . . . , εk, F0= (φ,Ω).

Lemma 1 ([7], p.179). The stochastic sequencek,Fk)k1 is a mar- tingale-difference.

(3)

Lemma 2. Let p(x) be the known positive continuously differentiable distribution density on [−π, π], and points xi be chosen from the relation Rxi

πp(u)du=ni, i= 1, n.

If NlnnN 0 forn→ ∞, then

EUnN =θ1+O

’NlnN n

“

, θ1= σ2 (2π)2

Z π

π

p1(u)du, (3) (2N+ 1)σnN2 →θ2= σ4

3 Z π

π

p2(u)du. (4)

Proof. From the definition ofxi we easily obtain

i= 1 np(xi)

”

1 +O1 n

‘•

,

whereO€1

n

is uniform with respect toi= 1, n.

Hence it follows that Qir= 1

n2p(xi)p(xr)KN(xi−xr)

”

1 +O1 n

‘•. (5)

Taking into account the relation

πmaxuπ|KN(u)|=O(N) (6)

and (5), we find

σnN2 = σ42(2N+1)2n2

Xn i=1

Xn j=1

KN2(xi−xj) 1

[p(xi)p(xj)]2+O1 n

‘. (7)

LetF(x) be a distribution function with density p(x) and Fn(x) be an empirical distribution function of the “sample”x1, x2, . . . , xn, i.e.,Fn(x) = n1Pn

k=1I(−∞,x)(xk), whereIA(·) is the indicator of the set A. Then the right side of (7) can be written as the integral

σnN2 = σ42(2N+ 1)2

Z π

π

Z π

π

KN2(t−s)dFn(t)dFn(s) [p(t)p(s)]2 +O1

n

‘.

(4)

Further we have

ŒŒ

ŒŒ Z π

π

Z π

π

KN2(t−s)dFn(t)dFn(s) [p(t)p(s)]2

Z π

π

Z π

π

KN2(t−s)dF(t)dF(s) [p(t)p(s)]2

ŒŒ

ŒŒ

≤I1+I2, I1=

ŒŒ

ŒŒ Z π

π

Z π

π

KN2(t−s) dFn(s) [p(t)p(s)]2

‚dFn(t)−dF(t)ƒŒŒŒŒ,

I2=

ŒŒ

ŒŒ Z π

π

Z π

π

KN2(t−s) dF(t) [p(t)p(s)]2

‚dFn(s)−dF(s)ƒŒŒŒŒ. By integration by parts in the internal integral inI1 we readily obtain

I12 Z π

π

dFn(s) p2(s)

Z π

π

ŒŒdFn(t)−dF(t)ŒŒŒŒ€KN0 (t−s)p(t)−

−KN(t−s)p0(t)

KN(t−s)/p3(t)ŒŒdt. (8) Since supπxπ|Fn(x)−F(x)|=O€1

n

and the relations [8]1

πmaxuπ|KN0 (u)|=O(N2), Z π

π

KN2(u)du= 2N+ 1, Z π

π|KN(u)|du=O(lnN)

(9)

are fulfilled, from (8) we have the estimate I1=O

’N2lnN n

“ . In the same manner we show that

I2=O

’N2lnN n

“ . Therefore

(2N+1)σ2nN= σ43

Z π

π

Z π

π

ΦN(s−t) dt ds p(s)p(t)+O

’NlnN n

“

, (10) where ΦN(u) =2N+1KN2(u) is the Fej´er kernel.

We shall complete the definition of the function p1 outside [−π, π] as regards its periodicity and also note that KN(u) and ΦN(u) are periodic functions with the period 2π. The continued function will be denoted by g(x). Then

Z π

π

Z π

π

ΦN(s−t) dt ds p(s)p(t) =

Z π

π

p2(x)dx+χn,

1See p. 115 in the Russian version of [8]: “Mir”, Moscow, 1965.

(5)

where

n| ≤ Z π

π¯N(x)−g(x)|dx,

¯ σN(x) =

Z π

π

ΦN(u)g(x−u)du.

Hence, on account of the theorem on convergence of the Fej´er integral

¯

σN(x) to g(x) in the norm of the spaceL1(−π, π) (see [9], p.481), we have χn 0 forn→ ∞.

Therefore

(2N+ 1)σ2nN σ43

Z π

π

p2(x)dx.

Now we shall prove (3). We have nN(x) =σ2

Xn j=1

1

np2(xj)KN2(x−xj)

”

1 +O1 n

‘•.

Applying the same reasoning as in deriving (10), we find nN(x) =σ2

n Z π

π

KN2(x−s) ds

p(s)+ON2lnN n2

‘. (11)

Therefore

EUnN = σ2 (2π)2

Z π

π

Z π

π

ΦN(t−s)ds dt

p(s) +ONlnN n

‘

=

= σ2 (2π)2

Z π

π

p1(s)ds+ONlnN n

‘ .

Denote by the symbold the convergence in distribution, and letξbe a random variable having normal distribution with zero mean and variance 1.

Theorem 1. Letxii= 1, nbe the same as in Lemma2and N2nlnN 0 forn→ ∞. Then, asnincreases,

2N+ 1(UnN−θ121/2d ξ.

Proof. We have

UnN−EUnN

σnN

=Hn(1)+Hn(2), where

Hn(1) = Xn j=1

ξj, Hn(2)= n 2π(2N+ 1)σnN

Xn i=1

2i −Eε2i)Qii.

(6)

Hn(2) converges to zero in probability. Indeed, DHn(2) n241

(2π)2(2N+ 1)2σ2nN Xn i=1

Q2ii=

= 41

(2π)2(2N+ 1)2σ2nN·n2 Xn i=1

1

(p(xi))4KN2(0)

’

1 +O1 n

‘“

≤C 1

nN2 =ON n

‘ , whence Hn(2) P

0. Here and in what follows C is the positive constant varying from one formula to another and the letter P above the arrow denotes convergence in probability.

We will now prove thatHn(1)

d ξ. To this end we will verify the validity of Corollaries 2 and 6 of Theorem 2 from [6]. We have to show whether the conditions contained in these statements are fulfilled for asymptotic normality of the square-integrable martingale-difference, which, by Lemma 1, is our sequencek,Fk}k1.

A direct calculation shows that Pn

k=1k2 = 1. Asymptotic normality will take place if forn→ ∞

Xn k=1

E‚

ξk2·I(|ξk| ≥ε)| Fk1

ƒ0 (12)

and

Xn k=1

ξ2kP 1. (13)

It is shown in [6] that the fulfillment of (13) and the condition sup

1knk|→P 0 implies the validy of (12) as well.

Since forε >0 Pˆ

sup

1knk| ≥ε‰

≤ε4 Xn k=1

4k,

to prove Hn(1) d

ξ we have to verify only (13) by the relation (15) to be given below.

We will establish Pn

k=1ξ2k P 1. For this it suffices to make sure that E(Pn

k=1ξk21))20 forn→ ∞, i.e., due toPn

i=1i2= 1 EXn

k=1

ξk2‘2

= Xn k=1

4k+ 2 X

1k1<k2n

k21ξk221. (14)

(7)

In the first place we find thatPn

k=14k 0 forn→ ∞. By virtue of the definitions ofξk andηij we write

Xn k=1

4k=L(1)n +L(2)n , where

L(1)n = n4

π4(2N+ 1)4σ4nN41(Eε414) Xn k=2

k1

X

j=1

Q4jk,

L(2)n = 3n4σ441 (2N+ 1)4σ4nNπ4

Xn k=2

kX1

j=1

Q2jk‘2

.

From (5) and (6) we obtain

|L(1)n |=C 1 n4N4σ4nN

Xn k=2

k1

X

j=1

KN4(xj−xk) [p(xj)p(xk)]4

h1 +O1 n

‘i

≤Cn2σnN4 =ON n

‘2‘

and also

|L(2)n |=C 1 n2N4σ4nN

Xn k=2

1 n

k1

X

j=1

KN2(xj−xk) p(xj)p(xk)

h1 +O1 n

‘i

2

≤C 1 n2N4σnN4

Xn k=1

1 n

k1

X

j=1

KN2(xj−xk)

2

=

=C 1

n2N4σ4nN Xn k=2

’Z π

π

KN2(xk−u) p2(u) dFn(u)

“2

≤C 1 n2N4σnN4

Xn k=2

šhKN2(xk−u)p1(u)dui2

+

+h Z π

π

KN2(xk−u)p2(u)d€

Fn(u)−F(u)i2›2

.

Hence, taking into account the relation (9) and the formula of integration by parts, we have|L(2)n |=O

1 n

‘. Therefore Xn

k=1

4k0 for n→ ∞. (15)

(8)

Let us now establish that 2P

1k1<k2nk21ξk22 1 for n→ ∞. The definition ofξi implies

ξk21ξ2k2kX11

i=1

ηik21‘kX21

i=1

ηik22‘

kX11

i=1

ηik21‘kX21

i6=s=1

ηik2ηsk2

‘ +

kX21

i=1

ηik22‘ kX11

s6=t=1

ηsk1ηtk1

‘

kX11

s6=t=1

ηsk1ηtk1

‘ kX21

k6=r=1

ηkk1ηrk2

‘

=

=Bk(1)1k2+Bk(2)1k2+Bk(3)1k2+B(4)k1k2. Therefore

2 X

1k1<k2n

2k1ξk22= X4 i=1

A(i)n , where

A(i)n = 2 X

1k1<k2n

EBk(i)1k2, i= 1,4.

In the first place we consider A(3)n . By the definition of ηij we obtain ik22ηsk1ηtk1 = 0,s6=t,k1< k2. Thus

A(3)n = 0. (16)

Let us derive an estimate ofA(2)n . Divide the sumEBk(2)1k2into two parts:

EB(2)k1k2 =

kX11 i=1

k1

X

r6=s=1

ik21ηrk2ηsk2+

kX11 i=1

kX21 r6=s=k1+1

2ik1ηrk2ηsk2.

The second term is equal to zero, since icannot coincide with r or withs andr6=s; in this caseEηik21ηrk2ηsk2 = 0, and2ik1ηrk2ηsk2 = 0 also in the first term each time except for the cases=k1 orr=k1.

Thus

EBk(2)1k2 = 2

kX11 i=1

E€

ηik21ηik2ηk1k2

.

Hence, using the definition of ηij and the inequality|Qij| ≤ CnN2 obtained from (5) and (6), we find

ŒŒEBk(2)1k2ŒŒ≤C 1 (2N+ 1)2σnN4

kX11 i=1

Q2ik1. (17)

(9)

Next, taking into account statement (4) of Lemma 2 and the definition ofσ2nN, from (17) we have

|A(2)n | ≤C n N2σnN4

Xn k1=2

kX11 i=1

Q2ik1≤C 1

nN2 =ON n

‘

. (18)

Consider nowA(4)n . By the definition ofηij we obtain A(4)n = 8n4

π4(2N+ 1)4σnN4 X

s<t<k1<k2

Qsk1Qsk2Qtk1Qtk2

≤C n4 N4σ4nN

hŒŒŒ X

s,t,k1,k2

Qsk1Qsk2Qtk1Qtk2

ŒŒ

Œ+ +ŒŒŒ X

k1,s,t

Q2k1sQ2k1tŒŒŒ+ŒŒŒ X

k1,s,t

Qk1tQstQk1sQss

ŒŒ

Œi

=

=C n4 N4σ4nN

‚|E1|+|E2|+|E3|ƒ

. (19)

According to (5) and (6) we write E1=n7 X

s,t,k1

KN(xs−xk1)KN(xt−xk1)×

× Z π

π

KN(xs−u)KN(xt−u)dFn(u) +ON2 n

‘ .

Hence, integrating by parts and taking into account (9), we obtain E1=n7

Z π

π

X

s,t,k1

KN(xs−xk1)KN(xt−xk1)×

KN(xs−u)KN(xt−u)p(u)du+ON4lnN n5

‘

. (20)

Applying the same operations three times, we represent (20) in the form E1=n4

Z π

π

Z π

π

Z π

π

Z π

π

KN(z−u)KN(z−t)KN(y−u)KN(y−t)×

×p(y)p(u)p(z)p(t)du dt dz dy+ON4lnN n5

‘

=

=ONln3N n4

‘

+ON4lnN n5

‘ .

(10)

Thus

n4

N4σ4nN|E1|=Oln3N N

‘

+ON2lnN n

‘

. (21)

Further, it is not difficult to show n4

N4σ4nN|E2|=ON2 n

‘,

n4

N4σnN4 |E3|=ON2 n

‘ .

(22)

Therefore (19), (21), and (22) imply A(4)n =ON2lnN

n

‘

+Oln3N N

‘

. (23)

Finally, we will show thatA(1)n 1 forn→ ∞. For this representA(1)n

in the formA(1)n =Q(1)n +Q(2)n , where Q(1)n = 2 X

k1<k2

kX11

i=1

ik21‘kX21

j=1

2ik2‘ ,

Q(2)n = 2 X

k1<k2

EBk(1)1k2 X

k1<k2

kX11

i=1

2ik1‘kX21

j=1

ik22‘‘

.

From the definition ofσ2nN it follows that Q(1)n = 1

Xn k=2

kX1

i=1

ik2‘2

, where

Xn k=2

kX1

i=1

ik2‘2

≤C n4 N4σ4nN

Xn k=2

kX1

i=1

Q2ik‘2

≤C 1

4nN =ON2 n

‘.

Therefore

Q(1)n = 1 +O€ N2/n

. (24)

Let us now show thatQ(2)n 0. Q(2)n can be written as Q(2)n = 2 X

k1<k2

hkX11

i=1

€cov(ηik21, η2ik2) + cov(η2ik1, η2k1k2)i .

(11)

But

2ik1ηik22≤C n4

N4σ4nNQ2ik1·Q2ik2

≤C 1 n4N4σnN4

€ max

πuπ|KN(u)|4

=O 1 n4σnN4

‘.

Similarly,2ij=O€

n2σnN2

. Therefore cov(η2ik1, η2ik2) =O 1

n4σ4nN

‘

. (25)

Further, sinceP

1k1<k2n(k11) =O(n3), (25) implies Q(2)n =ON2

n

‘

. (26)

Thus, according to (24) and (26)

A(1)n = 1 +O€ N2/n

. (27)

Combining the relations (16), (18), (23) and (27), we finally obtain EXn

k=1

ξ2k2

0 for n→ ∞. Therefore

UnN−EUnN

σnN

d ξ.

Further, due to Lemma 2,EUnN =θ1+O(NlnnN) and (2N+ 1)σnN2 →θ2, and hence we obtain

(2N+ 1)1/2(UnN−θ121/2d ξ.

Denote

TnN = n 2π(2N+ 1)

Z π

π

‚µnN(x)−µ(x)ƒ2

dx.

Theorem 2. Let xi,i= 1, n, be the same as in Lemma2 and the func- tion µ(x) with periodhave bounded derivatives up to the second order.

Moreover, if N2lnN/n 0 and nln2N/N9/2 0 for n → ∞, then

2N+ 1(TnN−θ121/2d ξ.

(12)

Before we proceed to proving the theorem, we have to show Z π

π|KN0 (u)|du=O(NlnN). (28) Denote Deν(u) =Pν

k=1sinku. Then by virtue of the Abel transformation we have

KN0 (u) = XN k=1

ksinku=

NX1 ν=1

Deν(u) +NDeN.

It is well known [8] that ην = (lnν)1Rπ

π|Deν(u)|du 1 for ν → ∞. DenotebN =PN1

ν=1 lnν. Then by the Toeplitz lemma RN = 1

bN NX1

ν=1

lnν·ην1.

Therefore Z π

π|KN0 (u)|du≤

NX1 ν=1

Z π

π|Deν(u)|du+N Z π

π|DeN(u)|du=

=bN·RN +N Z π

π|DeN(u)|du=O(NlnN).

Let us return to the proof of the theorem. We have TnN =UnN+A1n+A2n, A1n= n

π(2N+ 1) Z π

π

‚µnN(x)−EµnN(x)ƒ‚

nN(x)−µ(x)ƒ dx, A2n= n

2π(2N+ 1) Z π

π

‚nN(x)−µ(x)ƒ2

dx.

It is not difficult to find

2N+ 1E|A1n| ≤ 2

2N+ 1

Xn

j=1

2jh Z π

π

Kn(y−xj)×

׀

nN(y)−µ(x)

dyi2‘1/2

. But

nN(y) = Z π

π

µ(x) 1

p(x)KN(y−x)dFn(x)

1 +O€1 n

‘

(13)

and Z π

π

µ(x)p1(x)KN(y−x)dFn(x) =

= Z π

π

µ(x)KN(y−x) +O1 n

Z π

π|KN0 (u)|du‘ . It is well known ([10], p.22) that

Z π

π

µ(x)KN(y−x)dx=µ(y) +OlnN N2

‘

uniformly iny∈[−π, π]. By virtue of (28) this gives us nN(x) =µ(x) +OlnN

N2

‘

+ONlnN n

‘

. (29)

Therefore

2N+ 1E|A1n| ≤Cnln2N N9/2

‘1/2lnN N1/4 + +N2lnN

n

‘1/2ln3/2N

√N

i0. (30)

Further, from (29) we have

2N+ 1A2n≤Cnln2N N9/2 +N2

n ln2N

√N

‘

0. (31) Finally, the statement of Theorem 2 directly follows from Theorem 1, (30), and (31).

Using Theorems 1 and 2, it is easy to solve the problem concerning testing of the hypothesis onµ(x). Givenσ2, it is required to verify the hypothesis H0 : µ(x) = µ0(x). The critical region is defined approximately by the inequalityUnN≥dn(α) orTnN ≥dn(α), where

dn(α) =σ2€

L1+ (2N+ 1)1/2L2 λα, L1= ((2π)2

Z π

π

p1(x)dx, L2= 1 4π3

Z π

π

p2(x)dx‘1/2

, andλαis the quantile of levelαof standard normal distribution.

Let nowσ2 be unknown. We call an

N-consistent estimate of variance σ2, for instance,

S2n= 1 n

Xn i=1

€Yi−µ(xi2

,

where λ = λ(n) → ∞ is a sequence such that Nλ 0, Nlnλ42λ 0 and

N λ4

n 0 for n→ ∞.

(14)

Indeed, using the expressions (11) and (29), we easily find

√N(ESn2−σ2) =ON λ n

‘1/2‘

+ON1/2lnλ λ2

‘

. (32) Denote

Zj=Yj−Rj, Rj =

Xn k=1

YkkKλ(xj−xk).

Then

n2DSn2 = Xn j=1

DZj2+X

i6=i1

cov(Zi2, Zi21).

Simple calculations show that cov(Zj2, Zj21) =O

λ4 n

‘. ThereforeDSn2= O

λ4 n

‘

. This and (32) imply

N(Sn2−σ2)P 0.

Corollary. Let the conditions of Theorem 2 be fulfilled. Moreover, let

λ

n 0, N λn4 0 and Nlnλ42λ 0. Then Sn2L21

2N+ 1(UnN−Sn2L1)d ξ, Sn2L21

2N+ 1(TnN−Sn2L1)d ξ.

This corollary enables one to construct a test for verifying H0 :µ(x) = µ0(x). The critical region is defined approximately by the inequalityUnN den(α) or TnN den(α), where den(α) is obtained from dn(α) by using Sn2 instead ofσ2.

Consider now the local behavior of the test power in the case where the critical region is of the form {x R1, x ≥dn(α)}. More exactly, find a distribution of the quadratic functionalUnNunder a sequence of alternatives close to the hypothesisH0:µ(x) =µ0(x). The sequence is written as

H1: ¯µ(x) =µ0(x) +γnϕ(x) +o(γn), (33) whereγn0 appropriately and o(γn) is uniform in x∈[−π, π].

Theorem 3. Let µ¯n(x) satisfy the conditions of Theorem 2. If 2N + 1 = nδ, γn = n1/2+δ/4, 29 < δ < 12, then under the alternative H1

the statistic (2N + 1)1/2(UnN −θ1) is distributed in the limit normally

€1

Rπ

πϕ2(u)du, θ2

.

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Proof. Let us representUnN as the sum UnN = n

2π(2N+ 1) Z π

π

€µnN(x)−E1µnN(x)2

dx+

+ n

π(2N+ 1)γn

Z π

π

‚µnN(x)−E1µnN(x)ƒ e

ϕn(x)dx+

+ n

2π(2N+ 1)γn2 Z π

πϕe2n(x)dx=A1(n) +A2(n) +A3(n), whereE1(·) denotes the mathematical expectation under the hypothesisH1,

e ϕn(x) =

Xn j=1

ϕ(xj)∆jKn(x−xj).

Due to Theorem 1 one can readily assertain that

2N+ 1(A1(n)−θ1) is distributed asymptotically normal (0,

θ2).

By analogy with the proof of Lemma 2 we find

2N+ 1A3(n) = 1 2π

Z π

π

 Z π

π

ϕ(y)KN(x−y)dy‘2

dx+ON2lnN n

‘.

Hence, by virtue of theorem 2 from [9], p.474, we have

2N+ 1A3(n) 1 2π

Z π

π

ϕ2(u)du.

Further, for our choice ofN andγnwe can show by simple calculations that

2N+ 1E|A2(n)| ≤Cln2n

nδ/4 + lnn n17δ/4

‘ . Thus the local behaviour of the powerPH1(UnN≥dn(α)) is

PH1

€UnN ≥dn(α)

1֐

λα−θ21/2 1 2π

Z π

π

ϕ2(u)du‘

. (34) Since Rπ

πϕ2(u)du > 0 and is equal to zero iff ϕ(x) = 0, from (34) we conclude that the test for the hypothesis H0 : µ(x) = µ0(x) against alternatives of the form (33) is asymptotically strictly unbiased.

Remark. Similar results can be obtained by the same method for the kernel estimator of Priestley and Chao [1].

References

1. M.B. Priestley and M.T. Chao, Nonparametric function fitting. J.

Roy. Statist. Asoc. ser. B34(1972), 385-392.

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2. N.N. Chentsov, Estimation of the unknown distribution density by observations. (Russian)Dokl. Akad. Nauk SSSR147(1962), 45-48.

3. N.B. Smirnov and I.V. Dunin-Barkovskii, A course in probability theory and mathematical statistics for technical applications. (Russian) Nauka, Moscow,1969.

4. B.T. Polyak and A.V. Tsibakov, Asymptotic optimality of theCp-test in the projection estimation of the regression. (Russian)Teor. veroyatnost.

i primenen. 35(1990), No. 2, 305-317.

5. R.L. Eubank, J.D. Hart, and P. Speckman, Trigonometric series re- gression estimators with application to partially linear models. J. Multi- variate Anal. 32(1990), 70-83.

6. R.Sh. Liptser and A.N. Shiryayev, A functional central limit theorem for semimartingales. (Russian) Teor. veroyatnost. i primenen. 25(1980), No.4, 683-703.

7. E.A. Nadaraya, Nonparametric estimation of probability densities and regression curves. Kluwer Academic Publishers, Dordrecht, Holland,1989.

8. A. Zygmund, Trigonometric series, vol. 1. Cambridge University Press, Cambridge,1959.

9. A.N. Kolmogorov and S.V. Fomin, Elements of the theory of functions and functional analysis. (Russian)”Nauka”, Moscow,1989.

10. D. Jackson, The theory of approximation. American Mathematical Society, New York,1930.

(Received 1.07.1992) Author’s address:

Faculty of Mechanics and Mathamatics I.Javakhishvili Tbilisi State University 2 University St., 380043 Tbilisi Republic of Georgia

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