{"paper":{"title":"Weak lensing combined with the kinetic Sunyaev Zel'dovich effect: A study of baryonic feedback","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. Alarcon, A. Amon, A. A. Plazas Malagon, A. Campos, A. Carnero Rosell, A. Chen, A. Choi, A. Drlica-Wagner, A. Ferte, A. J. Ross, A. K. Romer, A. Navarro-Alsina, A. Pieres, A. Porredon, A. Roodman, A. Schneider, B. Flaugher, B. Yanny, B. Yin, C. Chang, C. Davis, C. Doux, C. Preston, C. Sanchez, C. To, D. Bacon, D. Brooks, D. Gruen, D. Huterer, D. J. James, D. L. Hollowood, D. Sanchez, D. Sanchez Cid, D. Sijacki, E. Bertin, E. Gaztanaga, E. M. Huff, E. Sanchez, E. Schaan, E. Sheldon, E. S. Rykoff, E. Suchyta, F. Andrade-Oliveira, F. J. Castander, F. Tarsitano, G. Giannini, G. Gutierrez, G. M. Bernstein, G. Tarle, H. Huang, H. T. Diehl, I. Ferrero, I. G. McCarthy, I. Harrison, I. Sevilla-Noarbe, I. Tutusaus, J. Annis, J. Blazek, J. Carretero, J. Cordero, J. DeRose, J. De Vicente, J. Elvin-Poole, J. Frieman, J. Garcia-Bellido, J. L. Marshall, J. McCullough, J. Mena-Fernandez, J. Muir, J. Myles, J. Prat, J. Salcido, J. Weller, J. Zuntz, K. Bechtol, K. Eckert, K. Herner, K. Honscheid, K. Kuehn, L. Bigwood, L. F. Secco, L. N. da Costa, M. Aguena, M. A. Troxel, M. Carrasco Kind, M. E. C. Swanson, M. E. S. Pereira, M. Gatti, M. Jarvis, M. Paterno, M. Raveri, M. R. Becker, M. Smith, M. Soares-Santos, M. Yamamoto, N. Battaglia, N. MacCrann, N. Weaverdyck, O. Alves, O. Friedrich, O. Lahav, P. Doel, P.-F. Leget, P. Wiseman, R. A. Gruendl, R. Cawthon, R. Chen, R. H. Wechsler, R. Miquel, R. P. Rollins, S. Allam, S. Bocquet, S. Desai, S. Dodelson, S. Everett, S. Ferraro, S. L. Bridle, S. Lee, S. Pandey, S. R. Hinton, S. Samuroff, T. Shin, W. G. Hartley, X. Fang, Y. Zhang","submitted_at":"2024-04-09T08:01:52Z","abstract_excerpt":"Extracting precise cosmology from weak lensing surveys requires modelling the non-linear matter power spectrum, which is suppressed at small scales due to baryonic feedback processes. However, hydrodynamical galaxy formation simulations make widely varying predictions for the amplitude and extent of this effect. We use measurements of Dark Energy Survey Year 3 weak lensing (WL) and Atacama Cosmology Telescope DR5 kinematic Sunyaev-Zel'dovich (kSZ) to jointly constrain cosmological and astrophysical baryonic feedback parameters using a flexible analytical model, `baryonification'. First, using "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2404.06098","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/2404.06098/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"}