Sensitivity of normality tests to non-normal data

In many statistical analyses, data need to be approximately normal or normally distributed. The Kolmogorov-Smirnov test, Anderson-Darling test, Cramer-von Mises test, and Shapiro-Wilk test are four statistical tests that are widely used for checking normality. One of the factors that influence these...

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Main Authors: Nor Aishah Ahad, Teh Sin Yin, Abdul Rahman Othman, Che Rohani Yaacob
Format: Article
Language:English
Published: Universiti Kebangsaan Malaysia 2011
Online Access:http://journalarticle.ukm.my/2511/
http://journalarticle.ukm.my/2511/
http://journalarticle.ukm.my/2511/1/15_NorAishah.pdf
id ukm-2511
recordtype eprints
spelling ukm-25112016-12-14T06:31:50Z http://journalarticle.ukm.my/2511/ Sensitivity of normality tests to non-normal data Nor Aishah Ahad, Teh Sin Yin, Abdul Rahman Othman, Che Rohani Yaacob, In many statistical analyses, data need to be approximately normal or normally distributed. The Kolmogorov-Smirnov test, Anderson-Darling test, Cramer-von Mises test, and Shapiro-Wilk test are four statistical tests that are widely used for checking normality. One of the factors that influence these tests is the sample size. Given any test of normality mentioned, this study determined the sample sizes at which the tests would indicate that the data is not normal. The performance of the tests was evaluated under various spectrums of non-normal distributions and different sample sizes. The results showed that the Shapiro-Wilk test is the best normality test because this test rejects the null hypothesis of normality test at the smallest sample size compared to the other tests, for all levels of skewness and kurtosis of these distributions. Universiti Kebangsaan Malaysia 2011-06 Article PeerReviewed application/pdf en http://journalarticle.ukm.my/2511/1/15_NorAishah.pdf Nor Aishah Ahad, and Teh Sin Yin, and Abdul Rahman Othman, and Che Rohani Yaacob, (2011) Sensitivity of normality tests to non-normal data. Sains Malaysiana, 40 (6). pp. 637-641. ISSN 0126-6039 http://www.ukm.my/jsm/
repository_type Digital Repository
institution_category Local University
institution Universiti Kebangasaan Malaysia
building UKM Institutional Repository
collection Online Access
language English
description In many statistical analyses, data need to be approximately normal or normally distributed. The Kolmogorov-Smirnov test, Anderson-Darling test, Cramer-von Mises test, and Shapiro-Wilk test are four statistical tests that are widely used for checking normality. One of the factors that influence these tests is the sample size. Given any test of normality mentioned, this study determined the sample sizes at which the tests would indicate that the data is not normal. The performance of the tests was evaluated under various spectrums of non-normal distributions and different sample sizes. The results showed that the Shapiro-Wilk test is the best normality test because this test rejects the null hypothesis of normality test at the smallest sample size compared to the other tests, for all levels of skewness and kurtosis of these distributions.
format Article
author Nor Aishah Ahad,
Teh Sin Yin,
Abdul Rahman Othman,
Che Rohani Yaacob,
spellingShingle Nor Aishah Ahad,
Teh Sin Yin,
Abdul Rahman Othman,
Che Rohani Yaacob,
Sensitivity of normality tests to non-normal data
author_facet Nor Aishah Ahad,
Teh Sin Yin,
Abdul Rahman Othman,
Che Rohani Yaacob,
author_sort Nor Aishah Ahad,
title Sensitivity of normality tests to non-normal data
title_short Sensitivity of normality tests to non-normal data
title_full Sensitivity of normality tests to non-normal data
title_fullStr Sensitivity of normality tests to non-normal data
title_full_unstemmed Sensitivity of normality tests to non-normal data
title_sort sensitivity of normality tests to non-normal data
publisher Universiti Kebangsaan Malaysia
publishDate 2011
url http://journalarticle.ukm.my/2511/
http://journalarticle.ukm.my/2511/
http://journalarticle.ukm.my/2511/1/15_NorAishah.pdf
first_indexed 2023-09-18T19:36:17Z
last_indexed 2023-09-18T19:36:17Z
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