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• W3102697983 endingPage "L8" @default.
• W3102697983 startingPage "L8" @default.
• W3102697983 abstract "The [CII] 158$mu$m fine-structure line is known to trace regions of active star formation and is the main coolant of the cold, neutral atomic medium. In this textit{Letter}, we report a strong detection of the [CII] line in the host galaxy of the brightest quasar known at $z>6.5$, the Pan-STARRS1 selected quasar PSO J036.5078+03.0498 (hereafter P036+03), using the IRAM NOEMA millimeter interferometer. Its [CII] and total far-infrared luminosities are $(5.8 pm 0.7) times 10^9 ,L_odot$ and $(7.6pm1.5) times 10^{12},L_odot$, respectively. This results in a $L_{[CII]} /L_{TIR}$ ratio of $sim 0.8times 10^{-3}$, which is at the high end for those found for active galaxies, though it is lower than the average found in typical main sequence galaxies at $zsim 0$. We also report a tentative additional line which we identify as a blended emission from the $3_{22} - 3_{13}$ and $5_{23} - 4_{32}$ H$_2$O transitions. If confirmed, this would be the most distant detection of water emission to date. P036+03 rivals the current prototypical luminous J1148+5251 quasar at $z=6.42$, in both rest-frame UV and [CII] luminosities. Given its brightness and because it is visible from both hemispheres (unlike J1148+5251), P036+03 has the potential of becoming an important laboratory for the study of star formation and of the interstellar medium only $sim 800,$Myr after the Big Bang." @default.
• W3102697983 created "2020-11-23" @default.
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• W3102697983 date "2015-05-18" @default.
• W3102697983 modified "2023-10-18" @default.
• W3102697983 title "BRIGHT [C II] 158 <i>μ</i> m EMISSION IN A QUASAR HOST GALAXY AT <i>z</i> = 6.54" @default.
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• W3102697983 doi "https://doi.org/10.1088/2041-8205/805/1/l8" @default.
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