Discovery of a radio-flaring M dwarf in a commensal transient search of the LADUMA field

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ID: 322897
2026
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Abstract
Abstract We report the discovery and characterisation of MKT J032848.4–271904.6, a new radio transient identified in the LADUMA field using SARAO Science Data Processor SDP UHF-band images from approximately one year of MeerKAT observations. Using the Transient Pipeline TraP and advanced filtering techniques, we identified a number of candidate variable radio sources in the field. All but one show variability consistent with refractive interstellar scintillation, leaving MKT J032848.4–271904.6 as the sole source exhibiting intrinsic variability. In addition, MKT J032848.4–271904.6 shows intrinsic variability at 0.816 GHz, with 13 radio detections across 41 epochs and a peak flux density of 1.041 ± 0.043 mJy. We associate this emission with a low-mass M-dwarf star LP 888–63, located 23 pc from the Sun and identified as a companion to the white dwarf binary system LAWD 14 WD 0326–273. LP 888–63 displays active flaring behaviour across the electromagnetic spectrum including multi-band optical data from MeerLICHT. TESS photometry reveals a periodic modulation in the blended light curve of 5.780 ± 0.507 days, consistent with rotational variability of a mid-M dwarf. Archival ESO spectra reveal Hα emission, confirming magnetic activity. These findings highlight the capability of MeerKAT’s SDP imaging and facilities like MeerLICHT for real-time detection and characterisation of stellar transients.
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Authors Moses Mlangeni, P. A. Woudt, Paul J Groot, Alex Andersson, Z N Khangale, F. Cavallaro, S. Bloemen, Paul Vreeswijk, D. A. H. Buckley, R. P. Fender, B. W. Stappers, D L A Pieterse, R Wijnands, Laura Driessen
Journal monthly notices of the royal astronomical society
Year 2026
DOI
10.1093/mnras/stag1420
URL
https://doi.org/10.1093/mnras/stag1420
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