| DOI | Resolve DOI: https://doi.org/10.1051/0004-6361/202140486 |
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| Author | Search for: Hutschenreuter, S.ORCID identifier: https://orcid.org/0000-0002-6952-9688; Search for: Anderson, C. S.; Search for: Betti, S.; Search for: Bower, G. C.; Search for: Brown, J.-A.; Search for: Brüggen, M.; Search for: Carretti, E.; Search for: Clarke, T.; Search for: Clegg, A.; Search for: Costa, A.; Search for: Croft, S.; Search for: Van Eck, C.; Search for: Gaensler, B. M.; Search for: De Gasperin, F.; Search for: Haverkorn, M.; Search for: Heald, G.; Search for: Hull, C. L. H.; Search for: Inoue, M.; Search for: Johnston-Hollitt, M.; Search for: Kaczmarek, J.1; Search for: Law, C.; Search for: Ma, Y. K.; Search for: MacMahon, D.; Search for: Mao, S. A.; Search for: Riseley, C.; Search for: Roy, S.; Search for: Shanahan, R.; Search for: Shimwell, T.; Search for: Stil, J.; Search for: Sobey, C.; Search for: O’Sullivan, S. P.; Search for: Tasse, C.; Search for: Vacca, V.; Search for: Vernstrom, T.; Search for: Williams, P. K. G.; Search for: Wright, M.; Search for: Enßlin, T. A. |
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| Affiliation | - National Research Council of Canada. Herzberg Astronomy and Astrophysics
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| Funder | Search for: European Research Council; Search for: Natural Sciences and Engineering Research Council of Canada; Search for: JSPS KAKENHI |
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| Format | Text, Article |
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| Subject | galaxy: general; ISM: magnetic fields; ISM: structure; galaxy: structure |
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| Abstract | Aims. This work provides an update to existing reconstructions of the Galactic Faraday rotation sky by processing almost all Faraday rotation data sets available at the end of the year 2020. Observations of extra-Galactic sources in recent years have further illuminated the previously underconstrained southern celestial sky, as well as parts of the inner disc of the Milky Way, along with other regions. This has culminated in an all-sky data set of 55 190 data points, thereby comprising a significant expansion on the 41 330 used in previous works. At the same time, this novelty makes an updated separation of the Galactic component a promising enterprise. The increased source density allows us to present our results in a resolution of about 1.3 × 10⁻² deg² (46.8 arcmin²), which is a twofold increase compared to previous works.
Methods. As for previous Faraday rotation sky reconstructions, this work is based on information field theory, namely, a Bayesian inference scheme for field-like quantities that handles noisy and incomplete data.
Results. In contrast to previous reconstructions, we find a significantly thinner and pronounced Galactic disc with small-scale structures exceeding values of several thousand rad m⁻². The improvements can mainly be attributed to the new catalog of Faraday data, but are also supported by advances in correlation structure modeling within numerical information field theory. We also provide a detailed discussion on the statistical properties of the Faraday rotation sky and we investigate correlations with other data sets. |
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| Publication date | 2022-01-04 |
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| Publisher | EDP Sciences |
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| In | |
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| Language | English |
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| Peer reviewed | Yes |
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| Identifier | aa40486-21 |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | 5f64da42-be8d-4416-97f8-c7a66d274820 |
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| Record created | 2024-02-19 |
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| Record modified | 2024-02-19 |
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