Non-LTE inversions of a confined X2.2 flare - I. The vector magnetic field in the photosphere and chromosphereG. J. M. Vissers, S. Danilovic, J. de la Cruz Rodríguez, J. Leenaarts, R. Morosin, C. J. Díaz Baso, A. Reid, J. Pomoell, D. J. Price and S. InoueA&A, 645 (2021) A1DOI: https://doi.org/10.1051/0004-6361/202038900