Radio activity from the rapidly rotating T dwarf 2MASS 2228-4310

dc.contributor.authorWandia, Kelvin
dc.contributor.authorGarrett, Michael A.
dc.contributor.authorGolden, Aaron
dc.contributor.authorHallinan, Gregg
dc.contributor.authorWilliams-Baldwin, David
dc.contributor.authorLucatelli, Geferson
dc.contributor.authorBeswick, Robert J.
dc.contributor.authorRadcliffe, Jack Frederick
dc.contributor.authorSiemion, Andrew
dc.contributor.authorMyburgh, Talon
dc.date.accessioned2026-04-02T07:03:37Z
dc.date.available2026-04-02T07:03:37Z
dc.date.issued2026-03
dc.descriptionDATA AVAILABILITY : Data underlying this article are publicly available in the NRAO data archive at https://data.nrao.edu/portal and can be accessed with project code 15A-045.
dc.description.abstractPlease read abstract in the article.
dc.description.departmentPhysics
dc.description.librarianhj2026
dc.description.sdgNone
dc.description.sponsorshipThis project has been made possible in part by a grant from the SETI Institute. This work made use of Astropy:3, a community-developed core python package and an ecosystem of tools and resources for astronomy (Astropy Collaboration 2013, 2018, 2022). The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France. This publication makes use of data products from the WISE, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration.
dc.description.urihttps://academic.oup.com/mnras
dc.identifier.citationKelvin Wandia, Michael A Garrett, Aaron Golden, Gregg Hallinan, David Williams-Baldwin, Geferson Lucatelli, Robert J Beswick, Jack F Radcliffe, Andrew Siemion, Talon Myburgh, Radio activity from the rapidly rotating T dwarf 2MASS 2228-4310, Monthly Notices of the Royal Astronomical Society, Volume 546, Issue 4, March 2026, stag085 pages 1-7, https://doi.org/10.1093/mnras/stag085.
dc.identifier.issn0035-8711 (print)
dc.identifier.issn1365-2966 (online)
dc.identifier.other10.1093/mnras/stag085
dc.identifier.urihttp://hdl.handle.net/2263/109423
dc.language.isoen
dc.publisherOxford University Press
dc.rights© The Author(s) 2026. Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/).
dc.subjectStars: brown dwarfs
dc.subjectStars: magnetic field
dc.subjectRadio continuum: stars
dc.titleRadio activity from the rapidly rotating T dwarf 2MASS 2228-4310
dc.typeArticle

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