{"paper":{"title":"Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Plazas Malag\\'on, A. Carnero Rosell, A. K. Romer, A. Mazoun, A. Pieres, A. Porredon, A. Tamosiunas, B. Flaugher, C. L. Reichardt, D. Brooks, D.Gr\\\"un, D. J. James, D. L. Hollowood, D. L. Tucker, D. Sanchez Cid, E. Sanchez, E. Suchyta, F. Andrade-Oliveira, G.Giannini, G.Gutierrez, G. Mahler, G. Tarle, H. Rubira, H. T. Diehl, I. Sevilla-Noarbe, J. Carretero, J. De Vicente, J.Frieman, J.Garcia-Bellido, J. J. Mohr, J. L. Marshall, J. Myles, J. Weller, K. Kuehn, L. E. Bleem, L. N. da Costa, M. Aguena, M. Carrasco Kind, M. Costanzi, M. E. C. Swanson, M. E. S. Pereira, M. Garny, M. Klein, M. Lima, M. Schubnell, M. Smith, N. Weaverdyck, O. Alves, O. Lahav, P. Doel, P. Wiseman, R.Gassis, R. L. C. Ogando, R. Miquel, S. Allam, S. Bocquet, S. Desai, S. Dodelson, S. Everett, S. Grandis, S. Lee, S.R.Hinton, S. Samuroff, S. W. Allen, T. M. Davis, T. Schrabback, V. Vikram","submitted_at":"2024-11-29T18:17:14Z","abstract_excerpt":"We use galaxy cluster abundance measurements from the South Pole Telescope (SPT) enhanced by Multi-Component Matched Filter (MCMF) confirmation and complemented with mass information obtained using weak-lensing data from Dark Energy Survey Year~3 (DES Y3) and targeted Hubble Space Telescope (HST) observations for probing deviations from the cold dark matter paradigm. Concretely, we consider a class of dark sector models featuring interactions between dark matter (DM) and a dark radiation (DR) component within the framework of the Effective Theory of Structure Formation (ETHOS). We focus on sce"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.19911","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/2411.19911/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"}