{"paper":{"title":"The miniJPAS survey: The role of group environment in quenching the star formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Cortesi, A. de Amorim, A. Ederoclite, A. Finoguenov, A. Hern\\'an-Caballero, A. J. Cenarro, A. Mar\\'in-Franch, C. L\\'opez-Sanjuan, C. Mendes de Oliveira, D. Crist\\'obal-Hornillos, E. P\\'erez, E. R. Carrasco, G. Mart\\'inez-Solaeche, H. V\\'azquez Rami\\'o, I. M\\'arquez, I. Pintos, J. A. Fern\\'andez-Ontiveros, J. Alcaniz, J. E. Rodr\\'iguez-Mart\\'in, J. M. Diego, J. M. V\\'ilchez, J. Varela, K. Taylor, L. A. D\\'iaz-Garc\\'ia, L. R. Abramo, L. Sodr\\'e Jr., M. Maturi, M. Moles, N. Ben\\'itez, P. A. A. Lopes, R. A. Dupke, R. Cid Fernandes, R. Garc\\'ia-Benito, R. M. Gonz\\'alez Delgado, S. Bonoli","submitted_at":"2022-07-12T18:00:13Z","abstract_excerpt":"The miniJPAS survey has observed $\\sim 1$ deg$^2$ on the AEGIS field with 60 bands (spectral resolution of $R \\sim 60$) in order to demonstrate the capabilities of the Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) that will map $\\sim 8000$ deg$^2$ of the northern sky in the next years. This paper shows the power of J-PAS to detect low mass groups and characterise their galaxy populations up to $z \\sim 1$. We use the spectral energy distribution fitting code BaySeAGal to derive the stellar population properties of the galaxy members in 80 groups at $z \\leq 0.8$ pr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2207.05770","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/2207.05770/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"}