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Related papers: Dust emission from the most distant quasars

200 papers

We present the results of new rest-frame far-IR observations of the z = 4.25 radio galaxy, 8C1435+635, which not only confirm that it contains an enormous quantity of dust (as first inferred from its mm-wave detection by Ivison 1995) but…

The detection of powerful near-infrared emission in high redshift (z>5) quasars demonstrates that very hot dust is present close to the active nucleus also in the very early universe. A number of high-redshift objects even show significant…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 C. Leipski , K. Meisenheimer

We use photometric data, from the optical to the mm for a large sample of optically selected radio-quiet quasars, at low and high redshifts, to test emission models from circum-nuclear dusty torii around them. Model parameters, such as dust…

Astrophysics · Physics 2007-05-23 P. Andreani , A. Franceschini , G. L. Granato

We have obtained high resolution (FWHM = 4.4 km/s) Keck spectra of images A and C of the gravitationally lensed QSO Q1422+231. The images are separated by 1.3" on the sky. In an absorption system at z = 3.538 gas column density variations…

Astrophysics · Physics 2007-05-23 Michael Rauch , Wallace L. W. Sargent , Thomas A. Barlow

We report on a dusty Mg~II absorber associated with the quasar SDSSJ003545.13+011441.2 (hereafter J0035+0114) at $z$=1.5501, which is the strongest one among the three Mg~II absorbers along the sight line of quasar. The two low redshift…

Cosmology and Nongalactic Astrophysics · Physics 2010-09-29 P. Jiang , J. Ge , J. X. Prochaska , V. P. Kulkarni , H. L. Lu , H. Y. Zhou

We present ALMA observations of the [C II] 158 micron fine structure line and dust continuum emission from the host galaxies of five redshift 6 quasars. We also report complementary observations of 250 GHz dust continuum and CO (6-5) line…

ALMA continuum measurements of the local ULIRG IRAS 07251-0248 E at 667$\mu$m reveal an extremely compact (R < 27 pc) and bright ($T_B$ >200 K) nucleus with an absorbing foreground envelope and a surrounding (R ~ 75 pc) disk or torus seen…

We present mid- and far-IR photometry of the high-redshift (z=4.69) dusty quasar BR1202-0725. The quasar was detected in the near-IR, at a flux level (0.7+/-0.2 mJy) consistent with an average Radio-Quiet Quasar at it's redshift. Only upper…

Astrophysics · Physics 2009-11-07 K. J. Leech , L. Metcalfe , B. Altieri

In order to test the unified scheme for luminous radio galaxies and quasars we observed 10 galaxy/quasar pairs from the 3CR catalogue with ISOPHOT at infrared wavelengths between 5 and 180 micron. Each pair was selected such that both the…

Astrophysics · Physics 2009-11-06 K. Meisenheimer , M. Haas , S. A. H. Müller , R. Chini , U. Klaas , D. Lemke

We present Karl G. Jansky Very Large Array (VLA) observations of 44 GHz continuum and CO J=2-1 line emission in BR1202-0725 at z=4.7 (a starburst galaxy and quasar pair) and BRI1335-0417 at z=4.4 (also hosting a quasar). With the full 8 GHz…

Astrophysics of Galaxies · Physics 2015-06-18 J. Wagg , C. L. Carilli , M. Aravena , P. Cox , L. Lentati , R. Maiolino , R. G. McMahon , D. Riechers , F. Walter , P. Andreani , R. Hills , A. Wolfe

We present the analysis of the absorption troughs of six outflows observed in quasar SDSS J1130+0411 ($z \approx 3.98$) with radial velocities ranging from $-2400$ to $-15,400$ km s$^{-1}$. These spectra were taken with the Very Large…

Astrophysics of Galaxies · Physics 2022-09-22 Andrew Walker , Nahum Arav , Doyee Byun

We report the first detection at 4.7 and 8.2 GHz with the RATAN-600 radio telescope of the source PSO J047.4478+27.2992, which has been announced as a blazar at z=6.1. The average flux density is $12\pm3$ and $8\pm4$ mJy at 4.7 and 8.2 GHz…

High Energy Astrophysical Phenomena · Physics 2020-12-15 T. Mufakharov , A. Mikhailov , Yu. Sotnikova , M. Mingaliev , V. Stolyarov , A. Erkenov , N. Nizhelskij , P. Tsybulev

We report on deep near-infrared F125W (J) and F160W (H) Hubble Space Telescope Wide Field Camera 3 images of the z=6.42 quasar J1148+5251 to attempt to detect rest-frame near-ultraviolet emission from the host galaxy. These observations…

We report the near-IR detection of a prominent CIV absorption in the rest-frame UV spectrum of the most distant known QSO, SDSS J104433.04-012502.2, at z=5.80. This QSO was recently observed with XMM-Newton and it was found to be notably…

Astrophysics · Physics 2009-11-06 R. Maiolino , F. Mannucci , C. Baffa , S. Gennari , E. Oliva

We present high spectral resolution VLT observations of the BAL quasar SDSS J0318-0600. This high quality data set allows us to extract accurate ionic column densities and determine an electron number density of n_e=10^3.3 +/- 0.2 cm^-3 for…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 Jay P. Dunn , Manuel A. Bautista , Nahum Arav , Maxwell Moe , Kirk T. Korista , Elisa Costantini , Chris Benn , Sara Ellison , Doug Edmonds

Absorption lines in the spectra of distant quasars whose sightlines pass through foreground galaxies provide a valuable tool to probe the dust and gas compositions of the interstellar medium (ISM) in galaxies. The first evidence of silicate…

Astrophysics of Galaxies · Physics 2014-05-05 Monique C. Aller , Varsha P. Kulkarni , Donald G. York , Daniel E. Welty , Giovanni Vladilo , Debopam Som

We use ALMA observations of the host galaxy of the quasar ULAS-J1342+0928 at z=7.54 to study the dust continuum and far infrared lines emitted from its interstellar medium. The Rayleigh-Jeans tail of the dust continuum is well sampled with…

We have measured mid-infrared radiation from an orientation-unbiased sample of 3CRR galaxies and quasars at redshifts 0.4 < z < 1.2 with the IRS and MIPS instruments on the Spitzer Space Telescope. Powerful emission (L_24micron > 10^22.4…

Astrophysics · Physics 2011-02-11 K. Cleary , C. R. Lawrence , J. A. Marshall , L. Hao , D. Meier

We present ALMA detections (or stringent upper limits) of the [CII] 158 $\mu m$ emission line and underlying dust continuum from five massive quenched galaxies (QGs) at 2<z<4.7. We find extreme variations in the molecular gas fractions…

Astrophysics of Galaxies · Physics 2026-04-13 C. D'Eugenio , E. Daddi , R. Gobat , S. Jin , D. Liu , H. Sun , F. Gentile , F. Bruckmann , Z. Liu , I. Delvecchio , L. Vallini , B. Magnelli , A. Zanella

We present the results from a $\sim500$ ks Chandra observation of the $z=6.31$ QSO SDSS J1030+0524. This is the deepest X-ray observation to date of a $z\sim6$ QSO. The QSO is detected with a total of 125 net counts in the full ($0.5-7$…