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相关论文: A search for HeH+ and CH in a high-redshift QSO

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We report the discovery of a new gravitationally lensed QSO, at a redshift z = 1.689, with four QSO components in a cross-shaped arrangement around a bright galaxy. The maximum separation between images is 2.6 arcsec, enabling a reliable…

天体物理学 · 物理学 2009-11-07 Lutz Wisotzki , Paul L. Schechter , Hale V. Bradt , Janine Heinmueller , Dieter Reimers

We present the selection of high-redshift ($z\gtrsim5.7$) radio-loud (RL) quasi-stellar object (QSO) candidates from the combination of the radio Rapid ASKAP Continuum Survey (RACS; at 888 MHz) and the optical/near-infrared Dark Energy…

星系天体物理 · 物理学 2022-12-28 L. Ighina , A. Caccianiga , A. Moretti , S. Belladitta , J. W. Broderick , G. Drouart , J. K. Leung , N. Seymour

This paper presents new optical and near-UV spectra of 11 extremely powerful jetted quasars, with radio to optical flux density ratio $>$ 10$^3$, that concomitantly cover the low-ionization emission of \mgii\ and \hb\ as well as the \feii\…

One of the surprises of the Herschel mission was the detection of ArH+ towards the Crab Nebula in emission and in absorption towards strong Galactic background sources. Although these detections were limited to the first quadrant of the…

星系天体物理 · 物理学 2020-11-11 Arshia M. Jacob , Karl M. Menten , Friedrich Wyrowski , Benjamin Winkel , David A. Neufeld

We report the detection of the satellite 18 cm OH lines at 1612 and 1720 MHz in the z=0.2467 molecular absorption system toward the radio source PKS 1413+135. The two OH lines are conjugate; the 1612 MHz line is seen in absorption while the…

天体物理学 · 物理学 2009-11-10 Jeremy Darling

We report on the discovery of a Type 1 quasar, SDSS 0956+5128, with a surprising combination of extreme velocity offsets. SDSS 0956+5128 is a broad-lined quasar exhibiting emission lines at three substantially different redshifts: a…

The intense UV radiation from a highly luminous QSO should excite fluorescent Ly-alpha emission from any nearby neutral hydrogen clouds. We present a very deep narrow-band search for such emission near the z=2.168 quasar PKS 0424-131,…

天体物理学 · 物理学 2011-03-10 Paul J. Francis , Joss Bland-Hawthorn

SDSS J092712.65+294344.0 has been proposed as a candidate for a supermassive black hole (~10^8.8 solar masses) ejected at high speed from the host galactic nucleus by gravitational radiation recoil, or alternatively for a supermassive black…

天体物理学 · 物理学 2011-02-11 G. A. Shields , E. W. Bonning , S. Salviander

We present results from 12 km/s resolution echelle spectroscopy of the bright $z=4.694$ QSO BR1202-0725. A preliminary analysis shows that high metallicity narrow line absorption clouds are present up to the redshift of the quasar. A damped…

天体物理学 · 物理学 2007-05-23 E. J. Wampler , G. M. Williger , J. A. Baldwin , R. F. Carswell , C. Hazard , R. G. McMahon

Hot, dust-obscured galaxies (Hot DOGs) are a population of hyper-luminous obscured quasars identified by WISE. We present ALMA observations of the [CII] fine-structure line and underlying dust continuum emission in a sample of seven of the…

We identify a horseshoe-shaped ring (HSR) of diffuse emission in J1407+0453 from the Faint Images of Radio Sky at Twenty-cm (FIRST) survey using the Very Large Array telescope. An optical galaxy SDSSJ140709.01+045302.1 is present near the…

星系天体物理 · 物理学 2024-03-20 Shobha Kumari , Sabyasachi Pal

We detected with the IRAM interferometer the lines of CO(4-3) and CO(9-8) from the recently-discovered broad absorption line quasar APM 08279+5255. The molecular lines are at a redshift of 3.911, which we take to be the true cosmological…

天体物理学 · 物理学 2009-10-31 D. Downes , R. Neri , T. Wiklind , D. J. Wilner , P. Shaver

We test the hypothesis whether high redshift QSOs would preferentially appear in small groups or pairs, and if they are associated with massive, young clusters. We carried out a photometric search for \Ly emitters on scales $\lesssim 10…

天体物理学 · 物理学 2009-11-07 L. Infante , J. Varela , M. Moles , G. Hertling , A. Garcia , F. Menanteau

Near-infrared images of the luminous, high redshift (z=2.1108) radio loud quasar 4C+09.17 reveal a complex structure. The quasar (K=15.76 mag) is surrounded by three "companion" objects having 17.9< K < 20.2 mag at radii of 1.7" < r < 2.9",…

天体物理学 · 物理学 2015-06-24 L. Armus , G. Neugebauer , M. D. Lehnert , K. Matthews

The Westerbork Synthesis Radio Telescope finds a weak 21cm line emission feature at the coordinates (RA-Dec-velocity) of the sub-Damped Lyman-alpha absorber observed at z_abs=0.00632 in the spectrum of PG1216+069. The emission feature,…

天体物理学 · 物理学 2009-11-11 F. H. Briggs , D. G. Barnes

We detect HCN J=5-4 emission from the ultraluminous quasar APM08279+5255 at z=3.911 using the IRAM Plateau de Bure interferometer. This object is strongly gravitationally lensed, yet still thought to be one of the most intrinsically…

天体物理学 · 物理学 2009-11-13 J. Wagg , D. J. Wilner , R. Neri , D. Downes , T. Wiklind

We present high angular resolution imaging of the quasar PSO J172.3556+18.7734 at $z=6.82$ with the Very Long Baseline Array (VLBA). This source currently holds the record of being the highest redshift radio-loud quasar. These observations…

We present results from two surveys for radio-loud quasars. These are (1) a northern survey reaching S(5GHz)=0.2Jy and (2) the Parkes QSO survey reaching S(2.7GHz)=0.25Jy, which together cover most of the sky. Both surveys use digitised…

天体物理学 · 物理学 2007-05-23 I. M. Hook , P. A. Shaver , R. G. McMahon

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

Observations of fluctuations in the redshifted 21 cm radiation from neautral hydrogen (HI) are perceived to be an important future probe of the universe at high redshifts. Under the assumption that at redshifts z less than 6…

天体物理学 · 物理学 2009-11-13 Sk. Saiyad Ali , Somnath Bharadwaj , Sanjay K. Pandey