{"paper":{"title":"Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: II. Anisotropic large-scale coherence in hot gas, galaxies, and dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Plazas Malag\\'on, A. Carnero Rosell, A. J. Duivenvoorden, A. Pieres, A. Porredon, A. Roodman, A. van Engelen, B. Santiago, C. Doux, C-H. To, C. Sif\\'on, D. Anbajagane, D. Bacon, D. Brooks, D. Gruen, D. J. James, D. L. Hollowood, D. Sanchez Cid, E. Baxter, E. Calabrese, E. Gaztanaga, E. J. Wollack, E. Sanchez, E. Suchyta, F. Menanteau, G. A. Marques, G. Giannini, G. Gutierrez, G. Tarle, I. Ferrero, I. Sevilla-Noarbe, J. Blazek, J. Carretero, J. De Vicente, J. Dunkley, J. Frieman, J. Garc\\'ia-Bellido, J. L. Marshall, J. Mena-Fern\\'andez, J. Myles, J. R. Bond, K. Honscheid, K. Kuehn, L. N. da Costa, M. Aguena, M. Costanzi, M. D. Niemack, M. E. C. Swanson, M. E. S. Pereira, M. Gatti, M. Lokken, M. Madhavacheril, M. Rodr\\'iguez-Monroy, M. Schubnell, M. Smith, N. Weaverdyck, O. Lahav, P. Doel, P. Wiseman, R. A. Gruendl, R. Hlo\\v{z}ek, R. Miquel, S. Bocquet, S. Desai, S. Everett, S. Lee, S. Pandey, S. R. Hinton, S. S. Allam, S. Samuroff, S. T. Staggs, V. Gluscevic, W. R. Coulton, Y. Guan, Z. Huang, Z. Li","submitted_at":"2024-09-06T18:01:23Z","abstract_excerpt":"Statistics that capture the directional dependence of the baryon distribution in the cosmic web enable unique tests of cosmology and astrophysical feedback. We use constrained oriented stacking of thermal Sunyaev-Zel'dovich (tSZ) maps to measure the anisotropic distribution of hot gas $2.5-40$ Mpc away from galaxy clusters embedded in massive filaments and superclusters. The cluster selection and orientation (at a scale of $\\sim15$ Mpc) use Dark Energy Survey (DES) Year 3 data, while expanded tSZ maps from the Atacama Cosmology Telescope Data Release 6 enable a $\\sim3\\times$ more significant m"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2409.04535","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/2409.04535/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"}