{"paper":{"title":"Milky Way Satellite Census. II. Galaxy--Halo Connection Constraints Including the Impact of the Large Magellanic Cloud","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. A. Plazas, A. B. Pace, A. Carnero Rosell, A. Drlica-Wagner, A. E. Evrard, A. H. Riley, A. Kravtsov, A. Palmese, A. R. Walker (DES Collaboration), B. Flaugher, B. Santiago, D. Brooks, D. Gruen, D. L. Burke, D. Thomas, D. W. Gerdes, E. Bertin, E. Gaztanaga, E. Krause, E. O. Nadler, E. Sanchez, E. Suchyta, F. Menanteau, F. Paz-Chinch\\'on, G. Green, G. Gutierrez, G. M. Bernstein, G. Tarle, J. Annis, J. Carretero, J. De Vicente, J. D. Simon, J. Frieman, J. Garc\\'ia-Bellido, J. Gschwend, J. L. Marshall, K. Bechtol, K. Honscheid, K. Kuehn, L. N. da Costa, M. A. G. Maia, M. Aguena, M. Carrasco Kind, M. Costanzi, M. McNanna, M. Smith, M. Soares-Santos, M. Y. Wang, N. Kuropatkin, O. Lahav, P. Fosalba, R. H. Wechsler, R. Miquel, S. Allam, S. Avila, S. Desai, S. Dodelson, S. Mau, S. R. Hinton, S. Serrano, T. M. C. Abbott, T. N. Varga, T. S. Li, V. Scarpine, W. G. Hartley, Y. -Y. Mao","submitted_at":"2019-12-06T19:01:07Z","abstract_excerpt":"The population of Milky Way (MW) satellites contains the faintest known galaxies and thus provides essential insight into galaxy formation and dark matter microphysics. Here we combine a model of the galaxy--halo connection with newly derived observational selection functions based on searches for satellites in photometric surveys over nearly the entire high Galactic latitude sky. In particular, we use cosmological zoom-in simulations of MW-like halos that include realistic Large Magellanic Cloud (LMC) analogs to fit the position-dependent MW satellite luminosity function. We report decisive e"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1912.03303","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/1912.03303/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"}