{"paper":{"title":"Physical properties of Lyman-alpha emitters at $z\\sim 0.3$ from UV-to-FIR measurements","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Bongiovanni, A. Cimatti, A. Ederoclite, A. M. P\\'erez Garc\\'ia, A. Poglitsch, B. Altieri, B. Magnelli, D. Elbaz, D. Lutz, E. Daddi, E. Le Floc'h, E. Sturm, F. Pozzi, H. Aussel, I. Oteo, I. Pintos-Castro, I. Valtchanov, J. Cepa, L. Riguccini, L. Tacconi, M. S\\'anchez-Portal, N. F\\\"orster Schreiber, P. Andreani, P. Popesso, R. Genzel, R. Maiolino, R. P\\'erez-Mart\\'inez, S. Berta","submitted_at":"2012-04-03T10:57:53Z","abstract_excerpt":"The analysis of the physical properties of low-redshift Ly$\\alpha$ emitters (LAEs) can provide clues in the study of their high-redshift analogues. At $z \\sim 0.3$, LAEs are bright enough to be detected over almost the entire electromagnetic spectrum and it is possible to carry out a more precise and complete study than at higher redshifts. In this study, we examine the UV and IR emission, dust attenuation, SFR and morphology of a sample of 23 GALEX-discovered star-forming (SF) LAEs at $z \\sim 0.3$ with direct UV (GALEX), optical (ACS) and FIR (PACS and MIPS) data. Using the same UV and IR lim"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1204.0782","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":""},"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"}