{"paper":{"title":"Herschel Far-IR counterparts of SDSS galaxies: Analysis of commonly used Star Formation Rate estimates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Bongiovanni, A. Ederoclite, A. M. P\\'erez Garc\\'ia, B. Magnelli, D. Lutz, F. Pozzi, G. Cresci, H. Dom\\'inguez S\\'anchez, I. Delvecchio, I. Oteo, J. Cepa, L. Riguccini, M. A. Lara-L\\'opez, M. S\\'anchez-Portal, P. Popesso, S. Berta","submitted_at":"2014-03-14T15:45:05Z","abstract_excerpt":"We study a hundred of galaxies from the spectroscopic Sloan Digital Sky Survey with individual detections in the Far-Infrared Herschel PACS bands (100 or 160 $\\mu$m) and in the GALEX Far-UltraViolet band up to z$\\sim$0.4 in the COSMOS and Lockman Hole fields. The galaxies are divided into 4 spectral and 4 morphological types. For the star forming and unclassifiable galaxies we calculate dust extinctions from the UV slope, the H$\\alpha$/H$\\beta$ ratio and the $L_{\\rm IR}/L_{\\rm UV}$ ratio. There is a tight correlation between the dust extinction and both $L_{\\rm IR}$ and metallicity. We calcula"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.3615","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"}