Milliarcsecond localization of the hyperactive repeating FRB 20220912A Article Swipe
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· 2024
· Open Access
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· DOI: https://doi.org/10.1093/mnras/stae632
We present very long-baseline interferometry (VLBI) observations of the hyperactive repeating FRB 20220912A using the European VLBI Network (EVN) outside of regular observing sessions (EVN-Lite). We detected 150 bursts from FRB 20220912A over two observing epochs in 2022 October. Combining the burst data allows us to localize FRB 20220912A to a precision of a few milliarcseconds, corresponding to a transverse scale of less than 10 pc at the distance of the source. This precise localization shows that FRB 20220912A lies closer to the centre of its host galaxy than previously found, although still significantly offset from the host galaxy’s nucleus. On arcsecond scales, FRB 20220912A is coincident with a persistent continuum radio source known from archival observations; however, we find no compact persistent emission on milliarcsecond scales. The 5σ upper limit on the presence of such a compact persistent radio source is 120 μJy, corresponding to a luminosity limit of (D/362.4 Mpc)$^2\, 1.8\times 10^{28}$erg s−1 Hz−1. The persistent radio emission is thus likely to be from star formation in the host galaxy. This is in contrast to some other active FRBs, such as FRB 20121102A and FRB 20190520B.
Related Topics
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1093/mnras/stae632
- https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stae632/56874105/stae632.pdf
- OA Status
- gold
- Cited By
- 18
- References
- 66
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4392503483
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4392503483Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1093/mnras/stae632Digital Object Identifier
- Title
-
Milliarcsecond localization of the hyperactive repeating FRB 20220912AWork title
- Type
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articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2024Year of publication
- Publication date
-
2024-03-05Full publication date if available
- Authors
-
D. M. Hewitt, Shivani Bhandari, B. Marcote, J. W. T. Hessels, Kenzie Nimmo, Franz Kirsten, U. Bach, Vladislavs Bezrukovs, Mohit Bhardwaj, Richard H. Blaauw, Justin D. Bray, S. Buttaccio, A. Corongiu, Marcin Gawroński, M. Giroletti, A. Keimpema, G. Maccaferri, Z. Paragi, M. Trudu, M. P. Snelders, T. Venturi, Na Wang, D. R. Williams, Nicholas Wrigley, Jun Yang, J. P. YuanList of authors in order
- Landing page
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https://doi.org/10.1093/mnras/stae632Publisher landing page
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https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stae632/56874105/stae632.pdfDirect link to full text PDF
- Open access
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YesWhether a free full text is available
- OA status
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goldOpen access status per OpenAlex
- OA URL
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https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stae632/56874105/stae632.pdfDirect OA link when available
- Concepts
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Physics, Fast radio burst, Galaxy, Astrophysics, Very-long-baseline interferometry, Luminosity, Offset (computer science), Radio galaxy, Astronomy, Programming language, Computer scienceTop concepts (fields/topics) attached by OpenAlex
- Cited by
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18Total citation count in OpenAlex
- Citations by year (recent)
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2025: 12, 2024: 6Per-year citation counts (last 5 years)
- References (count)
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66Number of works referenced by this work
- Related works (count)
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10Other works algorithmically related by OpenAlex
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