UHECR results of combined analyses of TA and Auger experiments

The origin of ultra-high-energy cosmic rays (UHECRs) is still unknown. Their sources are believed to be within the local universe (a few hundred megaparsecs), but deflections by intergalactic and Galactic magnetic fields prevent us from straightforwardly associating UHECRs their based on arrival directions, making angular distribution mostly isotropic. At higher energies, number potential source candidates both expected smaller, so available amount statistics. Hence, it interesting perform searches for anisotropies using several different energy thresholds. With a threshold 8 EeV dipole modulation has been discovered, with thresholds evidence mounting correlations certain nearby galaxies. Neither two main UHECR detectors, Pierre Auger Observatory Telescope Array project, full-sky coverage. Full-sky require combining datasets both, working group members collaborations tasked this. We present an overview challenges encountered in such analyses, recent results group, possible ways interpreting them, outlook near future.