Quasars as probes of the submillimetre cosmos at z>5: I. Preliminary SCUBA photometry
arXiv:astro-ph/0308132 · doi:10.1046/j.1365-8711.2003.07076.x
Abstract
We present submillimetre continuum observations of a sample of some of the highest redshift quasars currently known, made with the SCUBA bolometer array on the JCMT. The median redshift of the sample is 5.3. Two z>5 objects are strong (6 sigma) detections, with S(850um)>10mJy. A firm (5 sigma) detection is obtained for the z=5.7 quasar SDSS J1044-0125; and SDSS J1306+0356, at z=6.0, is detected with a signal-to-noise approx. 4. For the remainder of the sample we have obtained sensitive (sigma=1.5mJy) upper limits. Submm spectral indices measured for two of the sources are consistent with thermal reradiation from dust, rather than from synchrotron emission. Sensitive 450um upper limits imply that the dust is cool,suggesting large dust masses only 1Gyr after the Big Bang.
arXiv commentMNRAS Letters, accepted
References in corpus (29)
- A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
- The Demography of Massive Dark Objects in Galaxy Centres
- A Survey of z>5.8 Quasars in the Sloan Digital Sky Survey I: Discovery of Three New Quasars and the Spatial Density of Luminous Quasars at z~6
- Evidence for Reionization at z ~ 6: Detection of a Gunn-Peterson Trough in a z=6.28 Quasar
- A Survey of z>5.7 Quasars in the Sloan Digital Sky Survey II: Discovery of Three Additional Quasars at z>6
- A Redshift z = 6.56 Galaxy Behind the Cluster Abell 370
- The Discovery of a Luminous z=5.80 Quasar from the Sloan Digital Sky Survey
- Dust Formation In Early Galaxies
- SCUBA observations of galaxies with metallicity measurements: a new method for determining the relation between submm luminosity and dust mass
- A submillimetre survey of the star-formation history of radio galaxies
- High-redshift galaxies, their active nuclei and central black holes
- The Properties of Poor Groups of Galaxies: III. The Galaxy Luminosity Function
- Lyman Break Galaxies and the Star Formation Rate of the Universe at z~6
- High-Redshift Quasars Found in Sloan Digital Sky Survey Commissioning Data
- An excess of submm sources near 4C41.17: a candidate proto-cluster at z=3.8?
- A 250 GHz Survey of High Redshift QSOs from the Sloan Digital Sky Survey
- The SCUBA Bright Quasar Survey (SBQS): 850micron observations of the z>4 sample
- High-Redshift Quasars Found in Sloan Digital Sky Survey Commissioning Data VI. Sloan Digital Sky Survey Spectrograph Observations
- The far-infrared--submm spectral energy distribution of high-redshift quasars
- The SCUBA Bright Quasar Survey II: unveiling the quasar epoch at submillimetre wavelengths
- Submillimetre observations of luminous z>4 radio-quiet quasars and the contribution of AGN to the submm source population
- Gravitational Lensing of the SDSS High-Redshift Quasars
- High-Redshift Quasars Found in Sloan Digital Sky Survey Commissioning Data II: The Spring Equatorial Stripe
- Coupled spheroid and black-hole formation, and the multifrequency detectability of active galactic nuclei and submillimetre sources
- Discovery of a Color-Selected Quasar at z=5.50
- Five High-Redshift Quasars Discovered in Commissioning Imaging Data of the Sloan Digital Sky Survey
- An XMM-Newton detection of the z=5.80 X-ray weak quasar SDSSp J104433.04-012502.2
- A Chandra Search for X-Ray Jets in Redshift 6 Quasars
- Dust emission and star formation toward a redshift 5.5 QSO
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- Gemini Near-infrared Spectroscopy of Luminous z~6 Quasars: Chemical Abundances, Black Hole Masses, and MgII Absorption
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- A Herschel PACS and SPIRE study of the dust content of the Cassiopeia A supernova remnant
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- The dust mass in Cassiopeia A from a spatially resolved Herschel analysis
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- Probing the Evolution of IR Properties of z~6 Quasars: Spitzer Observations
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- Millimeter and Radio Observations of z~6 Quasars
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- Complete infrared spectral energy distributions of mm detected quasars at z>5
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- SCUBA2 High Redshift Bright Quasar Survey: Far-infrared Properties and Weak-line Features
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- The Growth of Black Holes and Their Host Spheroids in (Sub)mm-loud QSOs at High Redshift
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- A Direct Upper Limit on the Density of Cosmological Dust from the Absence of an X-ray Scattering Halo around the z=4.3 QSO 1508+5714
- The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light
- Dust Production Factories in the Early Universe: Formation of Carbon Grains in Red-supergiant Winds of Very Massive Population III Stars
- Heavily Reddened z~2 Type 1 Quasars II: H-alpha Star Formation Constraints from SINFONI IFU Observations
- Dust Models for the Extinction of Type IIn Supernova SN 2010jl
- The Circumgalactic Medium of Submillimeter Galaxies. II. Unobscured QSOs within Dusty Starbursts and QSO Sightlines with Impact Parameters below 100 Kiloparsec
- Radio recombination lines from obscured quasars with the SKA
- Sub-millimeter Detected z~2 Radio-quiet QSOs: Accurate Redshifts, Black Hole Masses, and Inflow/Outflow Velocities
- Inferring properties of dust in supernovae with neural networks
- Deep Submillimeter Observations of Two Lyman-alpha Emitting Galaxies at z~6.5