We report the detection of the 3P1 to 3P0 fine-structure line of neutral carbon in the z=4.12 quasar PSS 2322+1944, obtained at the IRAM Plateau de Bure interferometer. The CI 3P1-3P0 line is detected with a signal-to-noise ratio of about 6 with a peak intensity of about 2.5 mJy and a velocity-integrated line flux of 0.81+-0.12 Jy.km/s. Assuming an excitation temperature of 43 K (equal to the dust temperature), we derive a mass of neutral carbon (corrected for magnification) of about 1.2e7 Msun. In PSS 2322+1944, the cooling due to C is about 6 times smaller than for CO, whereas the CO and C cooling represents about 1e-4 of the far-infrared continuum and more than half of the cooling due to C+
5 pages, 3 figures, LaTex (l-aa.sty, psfig.sty), also available at http://www.ast.cam.ac.uk/~rgmWe r...
Together with C^+ and CO, C is an important reservoir of carbon in the interstellar medium. We prese...
Using the IRAM Plateau de Bure Interferometer, we report the detection of the 158 μm [C II] emission...
4 pages, 2 PostScript figures. Accepted for publication as a letter in Astronomy & Astrophysics. Use...
We report the detection of the $^3{\rm P}_1\to{}^3{\rm P}_0$ fine-structure line of neutral carbon ...
Using the IRAM 30 m telescope we detected the lower fine structure line of neutral carbon (CI(3P1...
We present the results of a search for cold gas at high redshift along quasar lines of sight carried...
Using the IRAM interferometer we have detected J=4-->3 and 5-- >4 CO line emission toward the radio ...
Using the IRAM 30 m telescope we detected the lower fine structure line of neutral carbon (C I$(\rm...
Using the IRAM interferometer we have detected $J=4{\rightarrow}3$ and $5{\rightarrow}4$ CO line em...
We present a survey of atomic carbon (C I) emission in high-redshift (z > 2) submillimeter galaxies ...
We present the first results of an Atacama Large Millimeter Array survey of the lower fine-structure...
Using the IRAM 30 m telescope and the Plateau de Bure interferometer we have detected the CI(^3P2 to...
5 pages, 2 figures, uses aa.cls and psfig.styWe present the results of a CO survey of gravitationall...
International audienceWe present the results of a search for cold gas at high redshift along quasar ...
5 pages, 3 figures, LaTex (l-aa.sty, psfig.sty), also available at http://www.ast.cam.ac.uk/~rgmWe r...
Together with C^+ and CO, C is an important reservoir of carbon in the interstellar medium. We prese...
Using the IRAM Plateau de Bure Interferometer, we report the detection of the 158 μm [C II] emission...
4 pages, 2 PostScript figures. Accepted for publication as a letter in Astronomy & Astrophysics. Use...
We report the detection of the $^3{\rm P}_1\to{}^3{\rm P}_0$ fine-structure line of neutral carbon ...
Using the IRAM 30 m telescope we detected the lower fine structure line of neutral carbon (CI(3P1...
We present the results of a search for cold gas at high redshift along quasar lines of sight carried...
Using the IRAM interferometer we have detected J=4-->3 and 5-- >4 CO line emission toward the radio ...
Using the IRAM 30 m telescope we detected the lower fine structure line of neutral carbon (C I$(\rm...
Using the IRAM interferometer we have detected $J=4{\rightarrow}3$ and $5{\rightarrow}4$ CO line em...
We present a survey of atomic carbon (C I) emission in high-redshift (z > 2) submillimeter galaxies ...
We present the first results of an Atacama Large Millimeter Array survey of the lower fine-structure...
Using the IRAM 30 m telescope and the Plateau de Bure interferometer we have detected the CI(^3P2 to...
5 pages, 2 figures, uses aa.cls and psfig.styWe present the results of a CO survey of gravitationall...
International audienceWe present the results of a search for cold gas at high redshift along quasar ...
5 pages, 3 figures, LaTex (l-aa.sty, psfig.sty), also available at http://www.ast.cam.ac.uk/~rgmWe r...
Together with C^+ and CO, C is an important reservoir of carbon in the interstellar medium. We prese...
Using the IRAM Plateau de Bure Interferometer, we report the detection of the 158 μm [C II] emission...