A MeerKAT search for persistent radio sources towards twenty-five localised Fast Radio Bursts

Fuente: arXiv
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Main Authors: Mfulwane, Lebogang L., Chibueze, James O., Letsele, Thulo P., Nyambe, Trevor M., Venter, Christo, Bezuidenhout, Mechiel Christiaan, Stappers, Benjamin W., Spitler, Laura G., Caleb, Manisha, Deller, Adam, Fortunato, Jéferson André Sales, Cornejo, Bernardo, Schüssler, Fabian, Ashkar, Halim, Bradascio, Frederica, Kalita, Surajit, Kundu, Anu, Kramer, Michael, Keane, Evan. F., Weltman, Amanda
Format: Preprint
Published: 2026
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author Mfulwane, Lebogang L.
Chibueze, James O.
Letsele, Thulo P.
Nyambe, Trevor M.
Venter, Christo
Bezuidenhout, Mechiel Christiaan
Stappers, Benjamin W.
Spitler, Laura G.
Caleb, Manisha
Deller, Adam
Fortunato, Jéferson André Sales
Cornejo, Bernardo
Schüssler, Fabian
Ashkar, Halim
Bradascio, Frederica
Kalita, Surajit
Kundu, Anu
Kramer, Michael
Keane, Evan. F.
Weltman, Amanda
author_facet Mfulwane, Lebogang L.
Chibueze, James O.
Letsele, Thulo P.
Nyambe, Trevor M.
Venter, Christo
Bezuidenhout, Mechiel Christiaan
Stappers, Benjamin W.
Spitler, Laura G.
Caleb, Manisha
Deller, Adam
Fortunato, Jéferson André Sales
Cornejo, Bernardo
Schüssler, Fabian
Ashkar, Halim
Bradascio, Frederica
Kalita, Surajit
Kundu, Anu
Kramer, Michael
Keane, Evan. F.
Weltman, Amanda
contents The discovery of persistent radio sources (PRSs) associated with repeating fast radio bursts (FRBs) has shed light on the immediate environments and possible progenitors of these FRBs. The confirmed PRSs may support the theory that FRB progenitors are compact central engines, whilst the non-detections suggest diversity of FRB's local environment. We perform a subarcsecond-resolution MeerKAT search at 1.28 GHz on 25 well-localised FRB positions provided by ASKAP and MeerTRAP. We detect 14 radio sources and provide flux upper limits for 12 non-detections (both these numbers include a source that was detected during two epochs of observation, and not detected during one epoch, adding up to 26). One radio source shows variability as seen in flux variations over three epochs of observation. Archival optical data reveal excesses in the direction of 13 detected radio sources. Similarly for four sources in the X-ray band, with one possibly being a high-energy signature of a radio galaxy core. Since we cannot definitively classify our detected radio sources as PRSs, future high-resolution observations with e-MERLIN will be required to resolve the radio emission and pronounce on the presence of compact PRSs associated with the 14 detected sources presented here.
format Preprint
id arxiv_https___arxiv_org_abs_2602_07716
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle A MeerKAT search for persistent radio sources towards twenty-five localised Fast Radio Bursts
Mfulwane, Lebogang L.
Chibueze, James O.
Letsele, Thulo P.
Nyambe, Trevor M.
Venter, Christo
Bezuidenhout, Mechiel Christiaan
Stappers, Benjamin W.
Spitler, Laura G.
Caleb, Manisha
Deller, Adam
Fortunato, Jéferson André Sales
Cornejo, Bernardo
Schüssler, Fabian
Ashkar, Halim
Bradascio, Frederica
Kalita, Surajit
Kundu, Anu
Kramer, Michael
Keane, Evan. F.
Weltman, Amanda
High Energy Astrophysical Phenomena
The discovery of persistent radio sources (PRSs) associated with repeating fast radio bursts (FRBs) has shed light on the immediate environments and possible progenitors of these FRBs. The confirmed PRSs may support the theory that FRB progenitors are compact central engines, whilst the non-detections suggest diversity of FRB's local environment. We perform a subarcsecond-resolution MeerKAT search at 1.28 GHz on 25 well-localised FRB positions provided by ASKAP and MeerTRAP. We detect 14 radio sources and provide flux upper limits for 12 non-detections (both these numbers include a source that was detected during two epochs of observation, and not detected during one epoch, adding up to 26). One radio source shows variability as seen in flux variations over three epochs of observation. Archival optical data reveal excesses in the direction of 13 detected radio sources. Similarly for four sources in the X-ray band, with one possibly being a high-energy signature of a radio galaxy core. Since we cannot definitively classify our detected radio sources as PRSs, future high-resolution observations with e-MERLIN will be required to resolve the radio emission and pronounce on the presence of compact PRSs associated with the 14 detected sources presented here.
title A MeerKAT search for persistent radio sources towards twenty-five localised Fast Radio Bursts
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2602.07716