{"paper":{"title":"Euclid: The selection of quiescent and star-forming galaxies using observed colours","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Cimatti, A. Humphrey, A.N. Taylor, A. Secroun, B. Garilli, B. Kubik, C.J. Conselice, C. Maraston, C. Padilla, C. Tortora, D.C. Masters, E. Franceschi, E. Maiorano, E. Rossetti, F. Hormuth, F.J. Castander, F. Pasian, F. Raison, F. Sureau, G. Congedo, G. Meylan, G. Polenta, G. Zamorani, H. Israel, I. Lloro, I. Tereno, J. Brinchmann, J. Carretero, J. Rhodes, J. Zoubian, K. Jahnke, L. Bisigello, L. Conversi, L. Corcione, L. Pozzetti, L. Valenziano, M. Bolzonella, M. Castellano, M. Frailis, M. Fumana, M. Kunz, M. Moresco, M. Poncet, M. Roncarelli, M. Sauvage, M.S. Cropper, M. Wetzstein, N. Auricchio, O. Le F\\`evre, O. Marggraf, P.-A. Duc, P.B. Lilje, P. Franzetti, P. Schneider, R. Cledassou, R. Kohley, R. Massey, R. Saglia, R. Toledo-Moreo, S. Andreon, S. Cavuoti, S. Dusini, S. Kermiche, S. Ligori, S. Mei, S. Paltani, S. Pires, S. Serrano, T. Kitching, U. Kuchner, V. Capobianco, V. Pettorino, Y. Mellier, Y. Wang","submitted_at":"2020-03-16T18:00:01Z","abstract_excerpt":"The Euclid mission will observe well over a billion galaxies out to $z\\sim6$ and beyond. This will offer an unrivalled opportunity to investigate several key questions for understanding galaxy formation and evolution. The first step for many of these studies will be the selection of a sample of quiescent and star-forming galaxies, as is often done in the literature by using well known colour techniques such as the `UVJ' diagram. However, given the limited number of filters available for the Euclid telescope, the recovery of such rest-frame colours will be challenging. We therefore investigate "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2003.07367","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/2003.07367/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"}