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Using photometric data from the Dark Energy Survey and the Wide-fieldInfrared Survey Explorer, we estimate photometric redshifts for 105 milliongalaxies using the nearest-neighbour algorithm. From such a large data base,151,244 clusters of galaxies are identified in the redshift range of 0.1<z<1.5based on the overdensity of the total stellar mass of galaxies within a givenphotometric redshift slice, among which 76,826 clusters are newly identifiedand 30,477 clusters have a redshift z>1. We cross-match these clusters withthose in the catalogues identified from the X-ray surveys and theSunyaev--Zel'dovich (SZ) effect by the Planck, South Pole Telescope and AtacamaCosmology Telescope surveys, and get the redshifts for 45 X-ray clusters and 56SZ clusters. More than 95 percent SZ clusters in the sky region havecounterparts in our catalogue. We find multiple optical clusters in the line ofsight towards about 15 percent of SZ clusters.

Clusters of galaxies up to z=1.5 identified from photometric data of the Dark Energy Survey and unWISE