Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4765
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dc.contributor.authorGupta, Shashikant-
dc.contributor.authorSaini, T.D.-
dc.date.accessioned2012-06-27T10:38:39Z-
dc.date.available2012-06-27T10:38:39Z-
dc.date.issued2011-08-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2011, Vol. 415, p. 2594-2599en
dc.identifier.issn0035-8711-
dc.identifier.issn1365-2966 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/4765-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractTwo new statistics, namely Δinline image and Δχ, based on the extreme value theory, were derived by Gupta et al. We use these statistics to study the direction dependence in the HST Key Project data, which provides one of the most precise measurements of the Hubble constant. We also study the non-Gaussianity in this data set using these statistics. Our results for Δinline image show that the significance of direction-dependent systematics is restricted to well below the 1σ confidence limit; however, the presence of non-Gaussian features is subtle. On the other hand, the Δχ statistic, which is more sensitive to direction dependence, shows direction dependence systematics to be at a slightly higher confidence level, and the presence of non-Gaussian features at a level similar to the Δinline image statistic.en
dc.language.isoenen
dc.publisherWiley Interscience for the RASen
dc.relation.urihttp://adsabs.harvard.edu/abs/2011MNRAS.415.2594Gen
dc.relation.urihttp://arxiv.org/abs/1105.4949en
dc.relation.urihttp://dx.doi.org/10.1111/j.1365-2966.2011.18882.xen
dc.rights2011 The authors & the Royal Astronomical Society.en
dc.subjectmethods: statisticalen
dc.subjectcosmological parametersen
dc.titleNon-Gaussianity and direction-dependent systematics in HST key project dataen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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