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Redshift ∼2.7 is not special comment on the Kolmogorov analysis of JWST deep survey galaxies

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dc.contributor.author Joseph, P
dc.date.accessioned 2025-10-28T08:27:01Z
dc.date.available 2025-10-28T08:27:01Z
dc.date.issued 2025-09
dc.identifier.citation Astronomy & Astrophysics, Vol. 701, A256 en_US
dc.identifier.issn 0004-6361
dc.identifier.uri http://hdl.handle.net/2248/8805
dc.description Open Access en_US
dc.description Open 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.abstract Galikyan 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.iso en en_US
dc.publisher EDP Sciences en_US
dc.relation.uri https://doi.org/10.1051/0004-6361/202555988
dc.rights © The Authors 2025
dc.subject Methods: data analysis en_US
dc.subject Methods: statistical en_US
dc.subject Galaxies: high-redshift en_US
dc.title Redshift ∼2.7 is not special comment on the Kolmogorov analysis of JWST deep survey galaxies en_US
dc.type Article en_US


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