{ "id": "1312.0684", "version": "v1", "published": "2013-12-03T02:15:05.000Z", "updated": "2013-12-03T02:15:05.000Z", "title": "ALMA will determine the spectroscopic redshift z>8 with FIR [O III] emission lines", "authors": [ "Akio K. Inoue", "Ikkoh Shimizu", "Yoichi Tamura", "Hiroshi Matsuo", "Takashi Okamoto", "Naoki Yoshida" ], "comment": "ApJL in press", "journal": "2014, ApJ, 780, L18", "doi": "10.1088/2041-8205/780/2/L18", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "We investigate the potential use of nebular emission lines in the rest-frame far-infrared (FIR) for determining spectroscopic redshift of z>8 galaxies with the Atacama Large Millimeter/sub-millimeter Array (ALMA). After making a line emissivity model as a function of metallicity, especially for the [O III] 88 micron line which is likely to be the strongest FIR line from H II regions, we predict the line fluxes from high-z galaxies based on a cosmological hydrodynamics simulation of galaxy formation. Since the metallicity of galaxies reaches at ~0.2 Zsun even at z>8 in our simulation, we expect the [O III] 88 micron line as strong as 1.3 mJy for 27 AB objects, which is detectable at a high significance by <1 hour integration with ALMA. Therefore, the [O III] 88 micron line would be the best tool to confirm the spectroscopic redshifts beyond z=8.", "revisions": [ { "version": "v1", "updated": "2013-12-03T02:15:05.000Z" } ], "analyses": { "keywords": [ "spectroscopic redshift", "micron line", "atacama large millimeter/sub-millimeter array", "line emissivity model", "nebular emission lines" ], "tags": [ "journal article" ], "publication": { "journal": "The Astrophysical Journal", "year": 2014, "month": "Jan", "volume": 780, "number": 2 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1267173, "adsabs": "2014ApJ...780L..18I" } } }