{"paper":{"title":"The final WaZP galaxy cluster catalog of the Dark Energy Survey and comparison with SZE data","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Carnero Rosell, A. Plazas Malag\\'on, B. Flaugher, B. Santiago, C. Benoist, D. Bacon, D. Brooks, D. James, D.L. Hollowood, E. Sanchez, E. Suchyta, F. Andrade-Oliveira, F.J. Castander, G. Giannini, G. Gutierrez, G. Tarle, I. Sevilla, J. Carretero, J. De Vicente, J. Frieman, J. Garcia-Bellido, J. Gschwend, J. Marshall, J. Mena-Fern\\'andez, J. Weller, K. Honscheid, K. Kuehn, K. Romer, L. Bleem, L. da Costa, M. Aguena, M. Costanzi, M.E. da Silva Pereira, M. Smith, N. Weaverdyck, O. Alves, P. Doel, P. Giles, R. Gruendl, R. Miquel, S. Allam, S. Desai, S. Dodelson, S. Everett, S. Hinton, S. Lee","submitted_at":"2025-07-07T18:00:06Z","abstract_excerpt":"In this work, we present and characterize the galaxy cluster catalog detected by the WaZP cluster finder, which is not based on red-sequence identification, on the full six years of observations of the Dark Energy Survey (DES-Y6). The full catalog contains over 400k detected clusters with richnesses, Ngals, above 5 and that reach redshifts up to 1.3. We also provide a version of the catalog where the observation depth and richness computation are homogenized to be used for cosmology, containing 33k rich (Ngals >25) clusters. We compare our results with the previous WaZP catalog obtained from t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2507.05360","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2507.05360/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}