collaborators

7 papers

astro-ph.HE2026

The flash-ionised SN Ibn 2025kzr: H-free CSM formed during a precursor outburst 55 days prior to explosion

S. de Wet, G. Leloudas, D. A. H. Buckley +33

Type Ibn supernovae (SNe) are a class of interacting SNe characterised by narrow helium lines in their spectra. We present an extensive observational dataset of the Type Ibn SN 202…

astro-ph.SR2026

X-ray counterparts to stellar MeerKAT Galactic-plane compact radio sources

O. D. Egbo, P. J. Groot, D. A. H. Buckley +5

Radio emission from magnetically active stars arises mainly from non-thermal processes and complements high-energy X-ray emission. Sensitive, wide-field radio and X-ray surveys now…

astro-ph.SR2026

The optical photometric and spectroscopic periodicities of the cataclysmic variable SRGt 062340.2-265751

J. Brink, D. A. H. Buckley, M. Veresvarska +10

We report on optical spectroscopic and photometric follow-up observations of the eROSITA discovered transient SRGt 062340.2-265751 and show that it displays the characteristics of…

astro-ph.HE2026

The odyssey of the black hole low mass X-ray binary GX339-4: Five years of dense multi-wavelength monitoring

E. Tremou, S. Corbel, R. Fender +15

We present the longest and the densest quasi-simultaneous radio, X-ray and optical campaign of the black hole low mass X-ray binary GX339-4, covering five years of weekly GX339-4 m…

astro-ph.SR2025

TESS and ground-based observations of WZ Sge-type dwarf novae in outburst

Y. Tampo, N. Kojiguchi, K. Isogai +30

Dwarf nova (DN) superoutbursts are accompanied by superhumps, which change their periods and profiles over a superoutburst. We present the TESS and ground-based observations of nin…

astro-ph.HE2025

DW Cnc: a micronova with a negative superhump and a flickering spin

M. Veresvarska, S. Scaringi, C. Littlefield +15

Magnetic accreting white dwarfs in cataclysmic variables have been known to show bursts driven by different physical mechanisms; however, the burst occurrence is much rarer than in…