{"paper":{"title":"Consistent lensing and clustering in a low-$S_8$ Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Alarcon, A. Amon, A. A. Plazas Malag\\'on, A. Campos, A. Carnero Rosell, A. Choi, A. Dvornik, A. Fert\\'e, A. H. Wright, A. J. Ross, A. Kannawadi, A. Navarro- Alsina, A. Pieres, A. Porredon, A. Roodman, B. Joachimi, B. Yin, C. Doux, C. Heymans, C. To, D. Bacon, D. Brooks, D. Gruen, D. Huterer, D. L. Burke, D. L. Hollowood, D. Thomas, D. W. Gerdes, E. M. Huff, E. Sanchez, E. Sheldon, E. Suchyta, F. J. Castander, F. Menanteau, F. Paz-Chinchon, G. Giannini, G. Gutierrez, G. Tarle, H. Hildebrandt, H. Hoekstra, H. Miyatake, H. Shan, H. T. Diehl, I. Ferrero, I. Sevilla-Noarbe, I. Tutusaus, J. Annis, J. Blazek, J. Carretero, J. de Jong, J. DeRose, J. De Vicente, J. Elvin-Poole, J. Frieman, J. Garc\\'ia-Bellido, J. Gschwend, J. J. Mohr, J. L. Marshall, J. Muir, J. Myles, J. P. Dietrich, J. Prat, K. Eckert, K. Herner, K. Honscheid, K. Kuehn, L. F. Secco, L. N. da Costa, M. A. G. Maia, M. Aguena, M. Asgari, M. A. Troxel, M. Bilicki, M. Costanzi, M. Crocce, M. E. C. Swanson, M. E. S. Pereira, M. Gatti, M. Lima, M. Rodriguez-Monroy, M. White, N. C. Robertson, N. Kuropatkin, N. MacCrann, O. Lahav, P. Doel, R. A. Gruendl, R. Cawthon, R. Chen, R. H. Wechsler, R. Miquel, R. Morgan, S. Allam, S. Bocquet, S. Desai, S. Everett, S. Huang, S. Lee, S. More, S. R. Hinton, S. Serrano, S. Yuan, T. Nishimichi, T. N. Varga, T. Shin, T. Trster, W. G. Hartley, Y. Zhang","submitted_at":"2022-02-15T14:24:42Z","abstract_excerpt":"We evaluate the consistency between lensing and clustering probes of large-scale structure based on measurements of projected galaxy clustering from BOSS combined with overlapping galaxy-galaxy lensing from three surveys: DES Y3, HSC Y1, and KiDS-1000. An intra-lensing-survey study finds good agreement between these lensing data. We model the observations using the Dark Emulator and fit the data at two fixed cosmologies: Planck, with $S_8=0.83$, and a Lensing cosmology with $S_8=0.76$. For a joint analysis limited to scales with $R>5.25h^{-1}$Mpc, we find that both cosmologies provide an accep"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2202.07440","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/2202.07440/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"}