{"paper":{"title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Clustering","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Alarcon, A. A. Plazas Malag\\'on, A. Carnero Rosell, A. Choi, A. Farahi, A. Fert\\'e, A. K. Romer, A. Palmese, A. Porredon, A. Roodman, A. R. Walker, B. Flaugher, B. Yanny, C. Chang, C. Conselice, Chun-Hao To, C. Lidman, C. Zhou, D. Anbajagane, David H. Weinberg, D. Bacon, D. Brooks, DES Collaboration: T. M. C. Abbott, D. Gruen, D. L. Hollowood, D. Sanchez Cid, D. Thomas, E. Krause, E. Rozo, E. Sanchez, E. S. Rykoff, E. Suchyta, F. Andrade-Oliveira, F. J. Castander, G. Giannini, G. Gutierrez, G. Tarle, H. Lin, H. T. Diehl, H.-Y. Wu, I. Harrison, I. Sevilla-Noarbe, J. Blazek, J. Carretero, J. Elvin-Poole, J. Esteves, J. Garc\\'ia-Bellido, J. J. Mohr, J. L. Marshall, J. McCullough, J. Mena-Fern, J. Muir, J. Myles, J. Prat, J. Weller, K. Honscheid, L. N. da Costa, M. Aguena, M. A. Troxel, M. Costanzi, M. Crocce, M. E. S. Pereira, M. Gatti, M. Lima, M. Paterno, M. R. Becker, M. Smith, M. Yamamoto, N. Jeffrey, N. Weaverdyck, O. Lahav, P. Doel, P. Giles, R. A. Gruendl, R. H. Wechsler, R. L. C. Ogando, R. Miquel, S. Avila, S. Bhargava, S. Bocquet, S. Desai, S. Dodelson, S. Everett, S. Grandis, S. Lee, S. R. Hinton, T. Jeltema, T. M. Davis, V. Vikram, Y. Zhang","submitted_at":"2025-03-17T18:28:21Z","abstract_excerpt":"Galaxy clusters provide a unique probe of the late-time cosmic structure and serve as a powerful independent test of the $\\Lambda$CDM model. This work presents the first set of cosmological constraints derived with ~16,000 optically selected redMaPPer clusters across nearly 5,000 $\\rm{deg}^2$ using DES Year 3 data sets. Our analysis leverages a consistent modeling framework for galaxy cluster cosmology and DES-Y3 joint analyses of galaxy clustering and weak lensing (3x2pt), ensuring direct comparability with the DES-Y3 3x2pt analysis. We obtain constraints of $S_8 = 0.864 \\pm 0.035$ and $\\Omeg"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2503.13632","kind":"arxiv","version":1},"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/2503.13632/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"}