{ "id": "1409.4413", "version": "v1", "published": "2014-09-15T20:00:04.000Z", "updated": "2014-09-15T20:00:04.000Z", "title": "First CO(17-16) emission line detected in a z > 6 quasar", "authors": [ "Simona Gallerani", "Andrea Ferrara", "Roberto Neri", "Roberto Maiolino" ], "comment": "6 pages, 4 figures, accepted for publication in MNRAS Letter", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "We report the serendipitous detection of the CO(17-16) emission line toward the quasar SDSSJ114816.64+525150.3 (J1148) at redshift z = 6.4 obtained with the Plateau de Bure Interferometer. The CO(17-16) line is possibly contaminated by OH+ emission, that may account for ~ 35 - 60% of the total flux observed. Photo-Dissociation and X-ray Dominated Regions (PDRs and XDRs) models show that PDRs alone cannot reproduce the high luminosity of the CO(17-16) line relative to low-J CO transitions and that XDRs are required. By adopting a composite PDR+XDR model we derive molecular cloud and radiation field properties in the nuclear region of J1148. Our results show that highly excited CO lines represent a sensitive and possibly unique tool to infer the presence of X-ray faint or obscured supermassive black hole progenitors in high-z galaxies.", "revisions": [ { "version": "v1", "updated": "2014-09-15T20:00:04.000Z" } ], "analyses": { "keywords": [ "emission line", "obscured supermassive black hole progenitors", "radiation field properties", "bure interferometer", "total flux" ], "tags": [ "journal article" ], "publication": { "doi": "10.1093/mnras/stu2031", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2014, "month": "Dec", "volume": 445, "number": 3, "pages": 2848 }, "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1317179, "adsabs": "2014MNRAS.445.2848G" } } }