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Aguilar, J. Choppin de Janvry, J. DeRose, J.E. Forero-Romero, J. Silber, K. Honscheid, L. Le Guillou, M. Ishak, M. Landriau, M. Manera, M. Schubnell, N. Palanque-Delabrouille, O. Lahav, P. Doel, R. Joyce, R. Kehoe, R. Miquel, R. Zhou, S. Ahlen, S. Ferraro, S. Gontcho A Gontcho, S. Heydenreich, S. Juneau, S. Nadathur, T. Claybaugh, T. Kisner, T. Zhang, U. Seljak, W. d'Assignies, W.J. Percival","submitted_at":"2025-11-22T17:32:47Z","abstract_excerpt":"The calibration of tomographic redshift distributions is essential for cosmological analysis of weak lensing data. In this work, we calibrate all four tomographic bins of the Hyper Suprime Camera (HSC) weak lensing catalog with the Dark Energy Spectroscopic Instrument (DESI) Data Release 1 and 2 using the clustering redshifts technique. We include z > 1.2 redshift sources such as emission line galaxies (ELG) and quasars (QSO) sources in our calibration, which were not available in the previous HSC calibration (Rau et al. 2022), allowing a complete calibration of all the redshift bins. 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