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Photometric redshift (photo-z) is a fundamental parameter formulti-wavelength photometric surveys, while galaxy clusters are importantcosmological probers and ideal objects for exploring the dense environmentalimpact on galaxy evolution. We extend our previous work on estimating photo-zand detecting galaxy clusters to the latest data releases of the Dark EnergySpectroscopic Instrument (DESI) imaging surveys, Dark Energy Survey (DES), andHyper Suprime-Cam Subaru Strategic Program (HSC-SSP) imaging surveys and makecorresponding catalogs publicly available for more extensive scientificapplications. The photo-z catalogs include accurate measurements of photo-z andstellar mass for about 320, 293, and 134 million galaxies with $r<23$, $i<24$,and $i<25$ in DESI DR9, DES DR2, and HSC-SSP PDR3 data, respectively. Thephoto-z accuracy is about 0.017, 0.024, and 0.029 and the general redshiftcoverage is $z<1$, $z<1.2$, and $z<1.6$, respectively for those three surveys.The uncertainties of the logarithmic stellar mass that is inferred from stellarpopulation synthesis fitting is about 0.2 dex. With the above photo-z catalogs,galaxy clusters are detected using a fast cluster-finding algorithm. A total of532,810, 86,963, and 36,566 galaxy clusters with the number of members largerthan 10 are discovered for DESI, DES, and HSC-SSP, respectively. Their photo-zaccuracy is at the level of 0.01. The total mass of our clusters are alsoestimated by using the calibration relations between the optical richness andthe mass measurement from X-ray and radio observations. The photo-z and clustercatalogs are available at ScienceDB(https://www.doi.org/10.11922/sciencedb.o00069.00003) and PaperData Repository(https://doi.org/10.12149/101089).

Photometric redshifts and Galaxy Clusters for DES DR2, DESI DR9, and HSC-SSP PDR3 Data