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Right Censoring Case

In document Dual φ -Divergence Estimates (Stránka 26-34)

5. Random Right Censoring

6.1. Right Censoring Case

This subsection presents some simulations for right censoring case discussed inSection 5. A sample is generated from exp1and an exponential censoring scheme is used; the censoring distribution is taken to be exp1/9that the proportion of censoring is 10%. To study the robustness properties of our estimators, 20% of the observations are contaminated by exp5.

The DφDE’s αφθ are calculated for samples of sizes 25, 50, 100, and 150, and the hole procedure is repeated 500 times. We can see fromTable 9that the DφDEs perform well under the model in terms of MSE and are an attractive alternative to the AMLE.

Table 10 shows the variation in coverage of nominal 95% asymptotic confidence intervals according to the sample size. Clearly, under coverage of the confidence intervals, the DφDEs have poor coverage probabilities due to the censoring effect. However, for small-and moderate-sized samples, the DφDEs associated toγ2 outperform the AMLE.

Under contamination the performances of our estimators decrease considerably. Such findings are evidences for the need for more adequate procedures for right-censored data Tables11and12.

Remark 6.1. In order to extract methodological recommendations for the use of an appropriate divergence, it will be interesting to conduct extensive Monte Carlo experiments for several divergences or investigate theoretically the problem of the choice of the divergence which leads to an “optimal”in some senseestimate in terms of efficiency and robustness, which would go well beyond the scope of the present paper. Another challenging task is how to choose the bootstrap weights for a given divergence in order to obtain, for example, an efficient estimator.

Table 6: Empirical coverage probabilities for the normal distribution,B1000.

γ n25 n50 n75 n100 n150 n200

−1 0.87 0.90 0.93 0.92 0.93 0.96

0 0.91 0.94 0.94 0.93 0.94 0.96

0.5 0.93 0.93 0.95 0.93 0.94 0.96

1 0.46 0.45 0.48 0.46 0.45 0.50

2 0.96 0.97 0.96 0.95 0.96 0.96

Table 7: Empirical coverage probabilities for the exponential distribution,B500.

γ n25 n50 n75 n100 n150 n200

−1 0.67 0.83 0.87 0.91 0.93 0.92

0 0.73 0.87 0.91 0.93 0.96 0.93

0.5 0.76 0.88 0.91 0.94 0.96 0.93

1 0.76 0.88 0.90 0.95 0.97 0.93

2 0.76 0.89 0.91 0.96 0.96 0.94

Appendix

This section is devoted to the proofs of our results. The previously defined notation continues to be used in the following.

Proof ofTheorem 3.1. Proceeding as 34 in their proof of the Argmax theorem, that is, Corollary 3.2.3, it is straightforward to show the consistency of the bootstrapped estimates

αφθ.

Remark A.1. Note that the proof techniques of Theorem 3.3are largely inspired by that of Cheng and Huang6and changes have been made in order to adapt them to our purpose.

Proof ofTheorem 3.3. Keep in mind the following definitions:

Gn:√

nPn−Pθ0,

Gn:√

nPn−Pn.

A.1

In view of the fact thatPθ0∂/∂αhθ, θ0 0, then a little calculation shows that

Gn

∂αhθ, θ0 Gn

∂αhθ, θ0

nPθ0

∂αh

θ,αφθ

∂αhθ, θ0

Gn

∂αhθ, θ0

∂αh

θ,αφθ Gn

∂αhθ, θ0

∂αh

θ,αφθ √

nPn

∂αh

θ,αφθ .

A.2

Table 8: Empirical coverage probabilities for the exponential distribution,B1000.

γ n25 n50 n75 n100 n150 n200

−1 0.70 0.79 0.90 0.91 0.92 0.91

0 0.76 0.84 0.91 0.92 0.93 0.92

0.5 0.78 0.85 0.93 0.94 0.94 0.93

1 0.78 0.87 0.94 0.94 0.95 0.94

2 0.78 0.88 0.95 0.95 0.96 0.95

Table 9: MSE of the estimates for the exponential distribution under right censoring.

γ n25 n50 n100 n150

−1 0.1088 0.0877 0.0706 0.0563

0 0.1060 0.0843 0.0679 0.0538

0.5 0.1080 0.0860 0.0689 0.0544

1 0.1150 0.0914 0.0724 0.0567

2 0.1535 0.1276 0.1019 0.0787

Table 10: Empirical coverage probabilities for the exponential distribution under right censoring.

γ n25 n50 n100 n150

−1 0.55 0.63 0.63 0.64

0 0.59 0.66 0.64 0.64

0.5 0.61 0.66 0.64 0.65

1 0.63 0.67 0.66 0.66

2 0.64 0.70 0.68 0.67

Table 11: MSE of the estimates for the exponential distribution under right censoring, 20% of contamina-tion.

γ n25 n50 n100 n150

−1 0.1448 0.1510 0.1561 0.1591

0 0.1482 0.1436 0.1409 0.1405

0.5 0.1457 0.1402 0.1360 0.1342

1 0.1462 0.1389 0.1332 0.1300

2 0.1572 0.1442 0.1338 0.1266

Table 12: Empirical coverage probabilities for the exponential distribution under right censoring, 20% of contamination.

γ n25 n50 n100 n150

−1 0.44 0.49 0.54 0.57

0 0.46 0.49 0.53 0.57

0.5 0.46 0.49 0.53 0.57

1 0.45 0.49 0.53 0.57

2 0.45 0.49 0.52 0.53

Consequently, we have the following inequality:

According to 23, Theorem 2.2 under condition A.4, we have G1 OoP

W1 in Pθ0 -probability. In view of the CLT, we haveG2 OPθ01. By applying a Taylor series expansion, we have

W1inPθ0-probability. An analogous argument yields that -probability. Finally,G50 based on3.3. In summary,A.3can be rewritten as follows:

inPθ0-probability. On the other hand, by a Taylor series expansion, we can write Pθ0

Clearly it is straightforward to combineA.7withA.6, to infer the following:

nSαφθ−θ0OoP

in Pθ0-probability, by considering again the consistency ofαφθand condition A.3and making use ofA.8to complete the proof of3.23. We next prove3.24. Introduce

H1:−Gn

By some algebra, we obtain

nPθ0

Therefore, we have established

nPθ0

inPθ0-probability. To analyze the left-hand side ofA.11, we rewrite it as

nPθ0

By a Taylor expansion, we obtain

nS in Pθ0-probability. Keep in mind that, under conditionA.3, the matrix S is nonsingular.

Multiply both sides of A.13 byS−1 to obtain3.24. An application of 23, Lemma 4.6,

under the bootstrap weight conditions, thus implies3.25. Using1, Theorem 3.2and37, Lemma 2.11, it easily follows that

sup

x∈Rd

Pθ0

n

αφθ−θ0

x

−PN0,Σ≤xoPθ01. A.14

By combining3.25andA.14, we readily obtain the desired conclusion3.27.

Acknowledgments

The authors are grateful to the referees, whose insightful comments helped to improve an early draft of this paper greatly. The authors are indebted to Amor Keziou for careful reading and fruitful discussions on the subject. They would like to thank the associate editor for comments which helped in the completion of this work.

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