Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8805
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dc.contributor.authorJoseph, P-
dc.date.accessioned2025-10-28T08:27:01Z-
dc.date.available2025-10-28T08:27:01Z-
dc.date.issued2025-09-
dc.identifier.citationAstronomy & Astrophysics, Vol. 701, A256en_US
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/8805-
dc.descriptionOpen Accessen_US
dc.descriptionOpen Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited-
dc.description.abstractGalikyan et al. (2025, A&A, 696, L21) reported a statistically significant change in galaxy spectral properties at redshift z ' 2.7 based on a Kolmogorov Stochasticity Parameter analysis of JWST spectroscopic data of galaxies. In this comment, we demonstrate that this result is critically driven by a single outlier in the dataset that was employed. This outlier arises from the use of a questionable redshift estimate for one spectrum. When the outlier is removed or the redshift is corrected, the claimed transition at z ' 2.7 disappears entirely. By independently reproducing the previous analysis, we demonstrate that the claimed feature is not a robust statistical signal, but an artefact of this anomalous data point.en_US
dc.language.isoenen_US
dc.publisherEDP Sciencesen_US
dc.relation.urihttps://doi.org/10.1051/0004-6361/202555988-
dc.rights© The Authors 2025-
dc.subjectMethods: data analysisen_US
dc.subjectMethods: statisticalen_US
dc.subjectGalaxies: high-redshiften_US
dc.titleRedshift ∼2.7 is not special comment on the Kolmogorov analysis of JWST deep survey galaxiesen_US
dc.typeArticleen_US
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