# Nonparametric smoothing for extremal quantile regression with heavy   tailed distributions

**Authors:** Takuma Yoshida

arXiv: 1903.03242 · 2019-03-21

## TL;DR

This paper develops a nonparametric method for estimating extremal quantiles in heavy-tailed distributions, addressing data sparsity issues and providing theoretical guarantees for the estimator's performance.

## Contribution

It introduces a novel estimator for extremal quantiles using extrapolation from intermediate quantiles, supported by asymptotic and extreme value theory.

## Key findings

- Estimator is asymptotically normal.
- Convergence rates are established.
- Simulation confirms estimator effectiveness.

## Abstract

In several different fields, there is interest in analyzing the upper or lower tail quantile of the underlying distribution rather than mean or center quantile. However, the investigation of the tail quantile is difficult because of data sparsity. In this paper, we attempt to develop nonparametric quantile regression for the extremal quantile level. In extremal quantile regression, there are two types of technical conditions of the order of convergence of the quantile level: intermediate order or extreme order. For the intermediate order quantile, the ordinary nonparametric estimator is used. On the other hand, for the extreme order quantile, we provide a new estimator by extrapolating the intermediate order quantile estimator. The performance of the estimator is guaranteed by asymptotic theory and extreme value theory. As a result, we show the asymptotic normality and the rate of convergence of the nonparametric quantile regression estimator for both intermediate and extreme order quantiles. A simulation is presented to confirm the behavior of the proposed estimator. The data application is also assessed.

## Full text

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## Figures

60 figures with captions in the complete paper: https://tomesphere.com/paper/1903.03242/full.md

## References

47 references — full list in the complete paper: https://tomesphere.com/paper/1903.03242/full.md

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Source: https://tomesphere.com/paper/1903.03242