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RMTable2023 and PolSpectra2023: Standards for Reporting Polarization and Faraday Rotation Measurements of Radio Sources

dc.contributor.authorVan Eck, Cameron
dc.contributor.authorGaensler, B M
dc.contributor.authorHutschenreuter, Sebastian
dc.contributor.authorLivingston, Jack
dc.contributor.authorMa, Yik Ki
dc.contributor.authorRiseley, Chris J
dc.contributor.authorThomson, Alec J. M.
dc.contributor.authorAdebahr, B
dc.contributor.authorBasu, A
dc.contributor.authorBirkinshaw, Mark
dc.contributor.authorEnßlin, T. A
dc.contributor.authorHeald, G
dc.contributor.authorMao, S A
dc.contributor.authorMcClure-Griffiths, Naomi
dc.date.accessioned2025-01-08T00:38:21Z
dc.date.available2025-01-08T00:38:21Z
dc.date.issued2023
dc.date.updated2024-01-14T07:15:42Z
dc.description.abstractFaraday rotation measures (RMs) have been used for many studies of cosmic magnetism, and in most cases having more RMs is beneficial for those studies. This has lead to the development of RM surveys that have produced large catalogs, as well as meta-catalogs collecting RMs from many different publications. However, it has been difficult to take full advantage of all of these RMs, as the individual catalogs have been published in many different places, and in many different formats. In addition, the polarization spectra used to determine these RMs are rarely published, limiting the ability to reanalyze data as new methods or additional observations become available. We propose a standard convention for RM catalogs, RMTable2023, and a standard for source-integrated polarized spectra of radio sources, PolSpectra2023. These standards are intended to maximize the value and utility of these data for researchers and to make them easier to access. To demonstrate the use of the RMTable2023 standard, we have produced a consolidated catalog of 55,819 RMs collected from 42 published catalogs.
dc.description.sponsorshipques de Strasbourg. The Canadian Initiative for Radio Astronomy Data Analysis (CIRADA) is funded by a grant from the Canada Foundation for Innovation 2017 Innovation Fund (Project 35999) and by the Provinces of Ontario, British Columbia, Alberta, Manitoba and Quebec, in collaboration with the National Research Council of Canada, the US National Radio Astronomy Observatory, and Australiaʼs Commonwealth Scientific and Industrial Research Organisation. The Dunlap Institute is funded through an endowment established by the David Dunlap family and the University of Toronto. C.J.R. acknowledges financial support from the ERC Starting Grant “DRANOEL,” No. 714245. S.H. acknowledges funding from the European Research Council (ERC) under the European Unionʼs Horizon 2020 research and innovation program (grant agreement No. 772663). B.A. acknowledges funding from the German Science Foundation DFG, within the Collaborative Research Center SFB1491 ”Cosmic Interacting Matters—From Source to Signal.”
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0067-0049
dc.identifier.urihttps://hdl.handle.net/1885/733731533
dc.language.isoen_AUen_AU
dc.provenanceOriginal content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
dc.publisherInstitute of Physics Publishing
dc.rights© 2023. The Author(s). Published by the American Astronomical Society.
dc.rights.licenseCreative Commons Attribution 4.0 International License
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.sourceAstrophysical Journal Supplement Series
dc.titleRMTable2023 and PolSpectra2023: Standards for Reporting Polarization and Faraday Rotation Measurements of Radio Sources
dc.typeJournal article
dcterms.accessRightsOpen Access
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage25
local.bibliographicCitation.startpage1
local.contributor.affiliationVan Eck, Cameron, College of Science, ANU
local.contributor.affiliationGaensler, B M, University of Toronto
local.contributor.affiliationHutschenreuter, Sebastian, Radboud University
local.contributor.affiliationLivingston, Jack, OTH Other Departments, ANU
local.contributor.affiliationMa, Yik Ki, College of Science, ANU
local.contributor.affiliationRiseley, Chris J, University of Bologna
local.contributor.affiliationThomson, Alec J. M., ATNF, CSIRO Space & Astronomy
local.contributor.affiliationAdebahr, B, Faculty of Physics and Astronomy
local.contributor.affiliationBasu, A, Max-Planck-Institut für Radioastronomie,
local.contributor.affiliationBirkinshaw, Mark, University of Bristol
local.contributor.affiliationEnßlin, T. A, Max Planck Institute for Astrophysics
local.contributor.affiliationHeald, G, CSIRO Astronomy and Space Science
local.contributor.affiliationMao, S A, Max-Planck-Institut fur Radioastronomie
local.contributor.affiliationMcClure-Griffiths, Naomi, College of Science, ANU
local.contributor.authoruidVan Eck, Cameron, u1131642
local.contributor.authoruidLivingston, Jack, u5559529
local.contributor.authoruidMa, Yik Ki, u1105408
local.contributor.authoruidMcClure-Griffiths, Naomi, u1000518
local.description.notesImported from ARIES
local.identifier.absfor510100 - Astronomical sciences
local.identifier.absseo280120 - Expanding knowledge in the physical sciences
local.identifier.ariespublicationa383154xPUB43072
local.identifier.citationvolume267
local.identifier.doi10.3847/1538-4365/acda24
local.identifier.scopusID2-s2.0-85166353771
local.publisher.urlhttps://iopscience.iop.org/
local.type.statusPublished Version
publicationvolume.volumeNumber267

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