{"paper":{"title":"The FMOS-COSMOS survey of star-forming galaxies at $z\\sim1.6$ VI: Redshift and emission-line catalog and basic properties of star-forming galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alvio Renzini, Annagrazia Puglisi, Anton. M. Koekemoer, Daichi Kashino, David Sanders, Emanuele Daddi, Francesco Valentino, Giulia Rodighiero, Jeyhan Kartaltepe, John D. Silverman, Nobuo Arimoto, Olivier Ilbert, Olivier Le F\\`evre, St\\'ephanie Juneau, Tohru Nagao","submitted_at":"2018-12-04T17:02:40Z","abstract_excerpt":"We present a new data release from the Fiber Multi-Object Spectrograph (FMOS)-COSMOS survey, which contains the measurements of spectroscopic redshift and flux of rest-frame optical emission lines (H$\\alpha$, [NII], [SII], H$\\beta$, [OIII]) for 1931 galaxies out of a total of 5484 objects observed over the 1.7 deg$^2$ COSMOS field. We obtained $H$-band and $J$-band medium-resolution ($R\\sim3000$) spectra with FMOS mounted on the Subaru telescope, which offers an in-fiber line flux sensitivity limit of $\\sim 1 \\times 10^{-17}~\\mathrm{erg~s^{-1}~cm^{-2}}$ for an on-source exposure time of five h"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.01529","kind":"arxiv","version":2},"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"}