High time resolution search for prompt radio emission from the long GRB 210419A with the Murchison Widefield Array Article Swipe
J Tian
,
G. E. Anderson
,
P. J. Hancock
,
J. C. A. Miller‐Jones
,
M. Sokołowski
,
N. A. Swainston
,
A. Rowlinson
,
A. Williams
,
D. L. Kaplan
,
N. Hurley‐Walker
,
John Morgan
,
N. D. R. Bhat
,
Daniel Ung
,
S. J. Tingay
,
K. W. Bannister
,
M. E. Bell
,
Bradley W. Meyers
,
M. Walker
·
YOU?
·
· 2022
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/stac1483
YOU?
·
· 2022
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/stac1483
We present a low-frequency (170–200 MHz) search for prompt radio emission associated with the long GRB 210419A using the rapid-response mode of the Murchison Widefield Array (MWA), triggering observations with the Voltage Capture System for the first time. The MWA began observing GRB 210419A within 89 s of its detection by Swift, enabling us to capture any dispersion delayed signal emitted by this gamma-ray burst (GRB) for a typical range of redshifts. We conducted a standard single pulse search with a temporal and spectral resolution of $100\, \mu$s and 10 kHz over a broad range of dispersion measures from 1 to $5000\, \text{pc}\, \text{cm}^{-3}$, but none were detected. However, fluence upper limits of 77–224 Jy ms derived over a pulse width of 0.5–10 ms and a redshift of 0.6 < z < 4 are some of the most stringent at low radio frequencies. We compared these fluence limits to the GRB jet–interstellar medium interaction model, placing constraints on the fraction of magnetic energy (ϵB ≲ [0.05–0.1]). We also searched for signals during the X-ray flaring activity of GRB 210419A on minute time-scales in the image domain and found no emission, resulting in an intensity upper limit of $0.57\, \text{Jy}\, \text{beam}^{-1}$, corresponding to a constraint of ϵB ≲ 10−3. Our non-detection could imply that GRB 210419A was at a high redshift, there was not enough magnetic energy for low-frequency emission, or the radio waves did not escape from the GRB environment.
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Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1093/mnras/stac1483
- https://academic.oup.com/mnras/article-pdf/514/2/2756/44147439/stac1483.pdf
- OA Status
- bronze
- Cited By
- 6
- References
- 176
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4281645238
All OpenAlex metadata
Raw OpenAlex JSON
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https://openalex.org/W4281645238Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1093/mnras/stac1483Digital Object Identifier
- Title
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High time resolution search for prompt radio emission from the long GRB 210419A with the Murchison Widefield ArrayWork title
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2022Year of publication
- Publication date
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2022-05-30Full publication date if available
- Authors
-
J Tian, G. E. Anderson, P. J. Hancock, J. C. A. Miller‐Jones, M. Sokołowski, N. A. Swainston, A. Rowlinson, A. Williams, D. L. Kaplan, N. Hurley‐Walker, John Morgan, N. D. R. Bhat, Daniel Ung, S. J. Tingay, K. W. Bannister, M. E. Bell, Bradley W. Meyers, M. WalkerList of authors in order
- Landing page
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https://doi.org/10.1093/mnras/stac1483Publisher landing page
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https://academic.oup.com/mnras/article-pdf/514/2/2756/44147439/stac1483.pdfDirect link to full text PDF
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YesWhether a free full text is available
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bronzeOpen access status per OpenAlex
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https://academic.oup.com/mnras/article-pdf/514/2/2756/44147439/stac1483.pdfDirect OA link when available
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Physics, Redshift, Astrophysics, Gamma-ray burst, Interstellar medium, GalaxyTop concepts (fields/topics) attached by OpenAlex
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6Total citation count in OpenAlex
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2025: 2, 2023: 2, 2022: 2Per-year citation counts (last 5 years)
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176Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| publication_date | 2022-05-30 |
| publication_year | 2022 |
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