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• W2141105013 endingPage "101" @default.
• W2141105013 startingPage "101" @default.
• W2141105013 abstract "We present new millimeter and radio observations of nine z~6 quasars discovered in deep optical and near-infrared surveys. We observed the 250 GHz continuum in eight of the nine objects and detected three of them. New 1.4 GHz radio continuum data have been obtained for four sources, and one has been detected. We searched for molecular CO (6-5) line emission in the three 250 GHz detections and detected two of them. We study the FIR and radio emission and quasar-host galaxy evolution with a sample of 18 z~6 quasars that are faint at UV/optical wavelengths (rest-frame 1450A magnitudes of m_1450ge20.2). The average FIR-to-AGN UV luminosity ratio of this faint quasar sample is about two times higher than that of the bright quasars at z~6 (m_1450<20.2). A fit to the average FIR and AGN bolometric luminosities of both the UV/optically faint and bright z~6 quasars, and the average luminosities of samples of submillimeter /millimeter-observed quasars at z~2 to 5, yields a relationship of L_{FIR} {L_{bol}}^{0.62}. Five of the 18 faint z~6 quasars have been detected at 250 GHz. These 250 GHz detections, as well as most of the millimeter-detected optically bright z~6 quasars, follow a shallower trend of L_{FIR} {L_{bol}}^{0.45} defined by the starburst-AGN systems in local and high-z universe. The millimeter continuum detections in the five objects and molecular CO detections in three of them reveal a few x10^8 M_sun of FIR-emitting warm dust and 10^10 M_sun of molecular gas in the quasar host galaxies. All these results argue for massive star formation in the quasar host galaxies, with estimated star formation rates of a few hundred M_sun yr^{-1}. Additionally, the higher FIR-to-AGN luminosity ratio found in these 250 GHz-detected faint quasars also suggests a higher ratio between star formation rate and supermassive black hole accretion rate than the UV/optically most luminous quasars at z~6." @default.
• W2141105013 created "2016-06-24" @default.
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• W2141105013 date "2011-08-23" @default.
• W2141105013 modified "2023-09-30" @default.
• W2141105013 title "FAR-INFRARED AND MOLECULAR CO EMISSION FROM THE HOST GALAXIES OF FAINT QUASARS AT<i>z</i>∼ 6" @default.
• W2141105013 cites W1583855478 @default.
• W2141105013 cites W1613124003 @default.
• W2141105013 cites W1619886093 @default.
• W2141105013 cites W1821429365 @default.
• W2141105013 cites W1968508625 @default.
• W2141105013 cites W1968718345 @default.
• W2141105013 cites W1971835767 @default.
• W2141105013 cites W1979253784 @default.
• W2141105013 cites W1980265098 @default.
• W2141105013 cites W1997434795 @default.
• W2141105013 cites W2001852248 @default.
• W2141105013 cites W2005354990 @default.
• W2141105013 cites W2007714429 @default.
• W2141105013 cites W2013064166 @default.
• W2141105013 cites W2014720123 @default.
• W2141105013 cites W2022549090 @default.
• W2141105013 cites W2023106241 @default.
• W2141105013 cites W2026631083 @default.
• W2141105013 cites W2027344788 @default.
• W2141105013 cites W2031615933 @default.
• W2141105013 cites W2037744399 @default.
• W2141105013 cites W2051090249 @default.
• W2141105013 cites W2055437312 @default.
• W2141105013 cites W2058890501 @default.
• W2141105013 cites W2062166036 @default.
• W2141105013 cites W2068860926 @default.
• W2141105013 cites W2077326407 @default.
• W2141105013 cites W2077944558 @default.
• W2141105013 cites W2083468542 @default.
• W2141105013 cites W2083868640 @default.
• W2141105013 cites W2086125693 @default.
• W2141105013 cites W2094564770 @default.
• W2141105013 cites W2099124298 @default.
• W2141105013 cites W2103849902 @default.
• W2141105013 cites W2104291306 @default.
• W2141105013 cites W2110294314 @default.
• W2141105013 cites W2119836155 @default.
• W2141105013 cites W2120984237 @default.
• W2141105013 cites W2125383073 @default.
• W2141105013 cites W2149063305 @default.
• W2141105013 cites W2149398194 @default.
• W2141105013 cites W2154748230 @default.
• W2141105013 cites W2158613310 @default.
• W2141105013 cites W2160556971 @default.
• W2141105013 cites W2161654647 @default.
• W2141105013 cites W2165299443 @default.
• W2141105013 cites W2166911340 @default.
• W2141105013 cites W2169817004 @default.
• W2141105013 cites W2951911578 @default.
• W2141105013 cites W2994936490 @default.
• W2141105013 cites W3098673717 @default.
• W2141105013 cites W3098694197 @default.
• W2141105013 cites W3099573144 @default.
• W2141105013 cites W3102225801 @default.
• W2141105013 cites W3102699381 @default.
• W2141105013 cites W3103463892 @default.
• W2141105013 cites W3103868583 @default.
• W2141105013 cites W3104389387 @default.
• W2141105013 cites W3104459078 @default.
• W2141105013 cites W3105531222 @default.
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• W2141105013 doi "https://doi.org/10.1088/0004-6256/142/4/101" @default.
• W2141105013 hasPublicationYear "2011" @default.
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