2025A&A...700A.130I

We present the most extensive high-time resolution multi-band campaign to date on the candidate transitional millisecond pulsar (tMSP) 3FGL J1544.6-1125 in the enigmatic sub-luminous disk state with coordinated observations from the radio to the X-ray band. While XMM-Newton and NuSTAR X-ray light curves exhibit the characteristic high and low-mode bimodality, the source's faintness prevents firm evidence from being obtained for similar bimodality in the ultraviolet and near-infrared light curves, which are presented here for the first time. A re-analysis of archival XMM-Newton/OM data revealed an optical flare without an X-ray counterpart, likely originating from the outer accretion disk or the companion star. During our observations, no radio emission was detected, with a 3σ flux density upper limit of ∼8 μJy at 6 GHz. While past works already reported radio variability in the source, this limit is a factor of ≳3.5 below the average value measured in 2019 under similar conditions, underscoring significant radio variability despite the relatively stable X-ray flux. Simultaneous optical light curves in five filters obtained with GTC/HiPERCAM revealed flickering and dipping activities that resemble the observed X-ray variability along with a reddening trend at lower fluxes. The latter is consistent with discrete mass ejections that disrupt the inner flow and reduce both X-ray and optical fluxes, thereby driving the high-to-low-mode switches. The observed reddening suggests a common origin for most optical and X-ray emission at the boundary region between the pulsar wind and the inner disk, as also supported by our modeling of the spectral energy distribution in the high mode. Overall, our findings reinforce the mini-pulsar nebula picture for tMSPs in the sub-luminous state and demonstrate how coordinated high-time resolution multi-wavelength campaigns are essential to understanding the physical processes governing rapid mode switches in these systems.