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相关论文: Probing the Evolution of IR Properties of z~6 Quas…

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We present sensitive near--infrared VLT ISAAC spectroscopic observations of the z=6.08 quasar SDSS J030331.40-001912.9. This QSO is more than a magnitude fainter than other QSOs at z~6 for which NIR spectroscopy has been obtained to date…

宇宙学与河外天体物理 · 物理学 2015-05-13 J. D. Kurk , F. Walter , X. Fan , L. Jiang , S. Jester , H. -W. Rix , D. A. Riechers

We have observed 13 z >= 4.5 QSOs using the Multiband Imaging Photometer for Spitzer, nine of which were also observed with the Infrared Array Camera. The observations probe rest wavelengths ~ 0.6-4.3 micron, bracketing the local minimum in…

天体物理学 · 物理学 2010-11-11 D. C. Hines , O. Krause , G. H. Rieke , X. Fan , M. Blaylock , G. Neugebauer

We assemble a catalogue of 488 spectroscopically confirmed very high ($z\geq5.00$) redshift quasars and report their near- ($ZYJHK_{s}/K$) and mid- (WISE W1234) infrared properties. 97\% of the VH$z$Q sample is detected in one or more NIR…

星系天体物理 · 物理学 2020-05-08 Nicholas P. Ross , Nicholas J. G. Cross

We have measured the mid-infrared radiation from an orientation-unbiased sample of powerful 3C RR galaxies and quasars using the IRS and MIPS instruments aboard the Spitzer Space Telescope. We fit the Spitzer data as well as other…

天体物理学 · 物理学 2007-07-30 Kieran Cleary , Charles R. Lawrence , Jason A. Marshall , Lei Hao , David Meier

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…

宇宙学与河外天体物理 · 物理学 2015-06-03 C. Leipski , K. Meisenheimer

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…

天体物理学 · 物理学 2011-02-11 K. Cleary , C. R. Lawrence , J. A. Marshall , L. Hao , D. Meier

We present broad band imaging observations obtained with the ``peak up'' imagers of the Spitzer Space Telescope Infrared Spectrograph (IRS) at wavelengths of 16micron and 22micron for a number of sources detected primarily at submillimeter…

We present millimeter and radio observations of 13 SDSS quasars at reshifts z~6. We observed eleven of them with the Max-Planck Millimeter Bolometer Array (MAMBO-2) at the IRAM 30m-telescope at 250 GHz and all of them with the Very Large…

The four-image gravitationally lensed quasar QSO 2237+0305 is microlensed by stars in the lens galaxy. The amplitude of microlensing variability can be used to infer the relative size of the quasar as a function of wavelength; this provides…

宇宙学与河外天体物理 · 物理学 2011-02-11 Eric Agol , Stephanie Gogarten , Varoujan Gorjian , Amy Kimball

We report observations of three SDSS z>6 QSOs at 250 GHz (1.2mm) using the 117-channel Max-Planck Millimeter Bolometer (MAMBO-2) array at the IRAM 30-meter telescope. J1148+5251 (z=6.41) and J1048+4637 (z=6.23) were detected with 250 GHz…

天体物理学 · 物理学 2009-11-07 F. Bertoldi , C. L. Carilli , P. Cox , X. Fan , M. A. Strauss , A. Beelen , A. Omont , R. Zylka

We present Spitzer Space Telescope photometry of 18 Sloan Digital Sky Survey (SDSS) quasars at 2.7 <= z <= 5.9 which have weak or undetectable high-ionization emission lines in their rest-frame ultraviolet (UV) spectra (hereafter weak-lined…

We present mid-infrared spectra and photometry of thirteen redshift 0.4<z<1 dust-reddened quasars obtained with Spitzer IRS and MIPS. We compare properties derived from their infrared spectral energy distributions (intrinsic AGN luminosity…

宇宙学与河外天体物理 · 物理学 2012-09-27 Tanya Urrutia , Mark Lacy , Henrik Spoon , Eilat Glikman , Andreea Petric , Bernhard Schulz

We present Spitzer Space Telescope data of four isolated white dwarfs that were previously known to harbor circumstellar gaseous disks. IRAC photometry shows a significant infrared excess in all of the systems, SDSS0738+1835, SDSS0845+2257,…

太阳与恒星天体物理 · 物理学 2015-06-04 Carolyn Brinkworth , Boris Gaensicke , Jon Girven , Don Hoard , Tom Marsh , Stephen Parsons , Detlev Koester

We report on submillimetre observations of three high redshift (z>6) quasars, made using the SCUBA camera on the JCMT. Only one of the sample was detected at 850um-- SDSS J1148+5251 (z=6.43). It was also detected (>3 sigma significance) at…

天体物理学 · 物理学 2009-11-10 Ian Robson , Robert Priddey , Kate Isaak , Richard McMahon

The Canada-France High-z Quasar Survey (CFHQS) is an optical survey designed to locate quasars during the epoch of reionization. In this paper we present the discovery of the first four CFHQS quasars at redshift greater than 6, including…

We identify and characterize a population of luminous dust poor quasars at 0<z<5, similar in photometric properties to the objects found at z>6 previously. This class of active galactic nuclei has been known to show little IR emission from…

宇宙学与河外天体物理 · 物理学 2015-06-17 Hyunsung David Jun , Myungshin Im

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…

天体物理学 · 物理学 2009-11-10 Robert S. Priddey , Kate G. Isaak , Richard G. McMahon , E. I. Robson , C. P. Pearson

We present near-infrared J and K-band spectra of the z = 6.4 quasar SDSS J114816.64+525150.3 obtained with the NIRSPEC spectrograph at the Keck-II telescope, covering the rest-frame spectral regions surrounding the C IV 1549 and Mg II 2800…

天体物理学 · 物理学 2009-11-10 A. J. Barth , P. Martini , C. H. Nelson , L. C. Ho

We analyse a sample of 85 luminous (log(nuLnu(3\um)/erg s-1)>45.5) quasars with restframe ~2-11 \um spectroscopy from AKARI and Spitzer. Their high luminosity allows a direct determination of the near-infrared quasar spectrum free from host…

We present Herschel far-infrared (FIR) observations of two sub-mm bright quasars at high redshift: SDSS J1148+5251 (z=6.42) and BR 1202-0725 (z=4.69) obtained with the PACS instrument. Both objects are detected in the PACS photometric…

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