The Universe Editorial Office would like to make the following correction regarding the Academic Editor listed for this published paper [1]. The originally listed Academic Editor, Gregory Vereshchagin, has been removed and replaced with the Editor-in-Chief of Universe, Lorenzo Iorio.
Following the publication, concerns were brought to the attention of the Editorial Office regarding a potential conflict of interest between the authors of this article and the original Academic Editor.
Adhering to our procedure, an investigation was completed by the Editorial Office, which confirmed a recent collaboration between an author and the Academic Editor that could be perceived as a conflict of interest and that was judged as not aligning with MDPI’s conflict of interest policy relating to the handling of Special Issue submissions (https://www.mdpi.com/special_issues_guidelines (accessed on 10 June 2024)).
The Editorial Office and the Editorial Board conducted a post-publication review of the article, which included a review of the peer process and of the final decision. The result of this review was that the peer-review was judged to be sound, and the accepted decision was considered to be appropriate. Consequently, the Editorial Office and the Editorial Board have decided that no revision of this article is necessary. However, the listed Academic Editor has been corrected.
The Editorial Office confirms that this change does not affect the scientific results.
The original publication has also been updated.
Reference
- Kim, V.; Umirbayeva, A.; Aimuratov, Y. Estimates of the Surface Magnetic Field Strength of Radio Pulsars. Universe 2023, 9, 334. [Google Scholar] [CrossRef]
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© 2024 by the author. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/).