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Commensal Transient Searches with MeerKAT in Gamma-Ray Burst and Supernova Fields

Abstract:
The sensitivity and field of view of the MeerKAT radio telescope provide excellent opportunities for commensal transient searches. We carry out a commensal transient search in supernova and short gamma-ray burst fields using methodologies established by S. I. Chastain et al. We search for transients in MeerKAT L-band images with integration times of 30 minutes, finding 13 variable sources. We compare these sources to the VLASS and RACS survey data, and examine possible explanations for the variability. Additionally, for one of these sources we examine archival Chandra ACIS data. We find that 12 of these sources are consistent with variability due to interstellar scintillation. The remaining source could possibly have some intrinsic variability. We also split the MeerKAT L band into upper and lower halves, and search for transients in images with an integration time of 8 s. We find a source with a duration of 8–16 s that is highly polarized at the lowest frequencies. This source is spatially coincident with a star detected by the Transiting Exoplanet Survey Satellite. We conclude that this source may be consistent with a stellar flare. Finally, we calculate accurate upper and lower limits on the transient rate using transient simulations.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-4357/ade70a

Authors


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Role:
Author
ORCID:
0000-0003-3507-335X
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Role:
Author
ORCID:
0000-0001-9149-6707
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Role:
Author
ORCID:
0000-0002-5936-1156
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Role:
Author
ORCID:
0000-0002-1195-7022
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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal More from this journal
Volume:
988
Issue:
2
Article number:
227
Publication date:
2025-07-28
Acceptance date:
2025-06-21
DOI:
EISSN:
1538-4357
ISSN:
0004-637X


Language:
English
Keywords:
Source identifiers:
3150527
Deposit date:
2025-07-28
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