{"paper":{"title":"The SAMI Galaxy Survey: Spatially Resolving the Main Sequence of Star Formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adam L. Schaefer, Amanda J. Moffett, Andrew Hopkins, Andrew W. Green, Angus Wright, Anne M. Medling, Barbara Catinella, Brent Groves, Caroline Foster, Chiara Tonini, Christoph Federrath, C. Jakob Walcher, Dan S. Taranu, Edoardo Tescari, Edward Taylor, Elise Hampton, Geraint F. Lewis, Gerald Cecil, Gregory Goldstein, I-Ting Ho, Jesse van de Sande, Jessica V. Bloom, Joss Bland-Hawthorn, J. S. Lawrence, Julia J. Bryant, Kenji Bekki, Lisa J. Kewley, Luca Cortese, Luke J. M. Davies, Matthew Colless, Matt S. Owers, Michael Goodwin, Michael J. Drinkwater, Nicholas Scott, Nuria P. F. Lorente, Richard McDermid, Robert Sharp, Samuel N. Richards, Sarah Brough, Sarah K. Leslie, Sarah M. Sweet, Scott M. Croom, Simon P. Driver, Tayyaba Zafar, Warrick J. Couch","submitted_at":"2018-01-12T19:00:21Z","abstract_excerpt":"We present the ~800 star formation rate maps for the SAMI Galaxy Survey based on H{\\alpha} emission maps, corrected for dust attenuation via the Balmer decrement, that are included in the SAMI Public Data Release 1. We mask out spaxels contaminated by non-stellar emission using the [O III]/H{\\beta}, [N II]/H{\\alpha}, [S II]/H{\\alpha}, and [O I]/H{\\alpha} line ratios. Using these maps, we examine the global and resolved star-forming main sequences of SAMI galaxies as a function of morphology, environmental density, and stellar mass. Galaxies further below the star-forming main sequence are more"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.04283","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"}