094405

J1910-4410 is only the second confirmed white-dwarf pulsar after AR Sco. Tofully characterize the new system we are planning a coordinatedmulti-wavelength observational campaign from radio to X-ray wavelengthsinvolving MeerKAT the NTT with ULTRACAM the SAAO 1.9m with HIPPO andXMM-Newton which shall take place in October 2024. With the new data we want togain deeper understanding of the r^ant radiation mechanisms establish along-term ephemeris and determine the spin-down characterize the X-ray spectrumto distinguish between accretion-induced thermal and magnetospheric non-thermalcomponents to search for X-ray variability on long timescales and finallyestablish the phase relation between the broad and the narrow pulses. [truncated! Please see actual data for full text]