{"paper":{"title":"Dark Energy Survey Year 3 Results: Galaxy clustering and systematics treatment for lens galaxy samples","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Amon, A. A. Plazas Malag\\'on, A. Carnero Rosell, A. Choi, A. Fert\\'e, A. J. Ross, A. Palmese, A. Pieres, A. Porredon, A. Roodman, B. Flaugher, B. Jain, C. Conselice, C. J. Miller, C. To, D. Bacon, D. Brooks, D. Gruen, D. Huterer, D. J. James, D. L. Burke, D. L. Hollowood, D. Sanchez Cid, D. Thomas, E. Baxter, E. Bertin, E. Gaztanaga, E. Krause, E. L. Wagoner, E. M. Huff, E. Rozo, E. Sanchez, E. S. Rykoff, E. Suchyta, F. Andrade-Oliveira, F. J. Castander, F. Menanteau, F. Paz-Chinch\\'on, G. Giannini, G. Gutierrez, G. M. Bernstein, G. Tarle, H. Camacho, H. T. Diehl, I. Ferrero, I. Sevilla-Noarbe, J. Annis, J. Blazek, J. Carretero, J. DeRose, J. De Vicente, J. Elvin-Poole, J. Frieman, J. Garc\\'ia-Bellido, J. Gschwend, J. J. Mohr, J. L. Marshall, J. Mena-Fern\\'andez, J. Muir, J. Prat, K. Bechtol, K. Herner, K. Honscheid, K. Kuehn, L. N. da Costa, M. A. G. Maia, M. Aguena, M. Carrasco Kind, M. Costanzi, M. Crocce, M. E. S. Pereira, M. Jarvis, M. Lima, M. March, M. Rodr\\'iguez-Monroy, M. Smith, M. Soares-Santos, M. Tabbutt, N. Kuropatkin, N. MacCrann, N. Weaverdyck, O. Friedrich, P. Fosalba, P. Melchior, R. A. Gruendl, R. Cawthon, R. H. Wechsler, R. Miquel, R. Morgan, R. Rosenfeld, S. Allam, S. Avila, S. Bhargava, S. Desai, S. Dodelson, S. Everett, S. Pandey, S. R. Hinton, S. Serrano, T. Giannantonio, T. N. Varga (DES Collaboration), V. Scarpine, W. G. Hartley, X. Fang, Y. Park","submitted_at":"2021-05-28T01:58:49Z","abstract_excerpt":"In this work we present the galaxy clustering measurements of the two DES lens galaxy samples: a magnitude-limited sample optimized for the measurement of cosmological parameters, MagLim, and a sample of luminous red galaxies selected with the redMaGiC algorithm. MagLim / redMaGiC sample contains over 10 million / 2.5 million galaxies and is divided into six / five photometric redshift bins spanning the range $z\\in[0.20,1.05]$ / $z\\in[0.15,0.90]$. Both samples cover 4143 deg$^2$ over which we perform our analysis blind, measuring the angular correlation function with a S/N $\\sim 63$ for both s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2105.13540","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/2105.13540/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"}