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相关论文: Q0906+6930: The Highest-Redshift Blazar

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The radio-loud quasar SDSS J102623.61+254259.5, at a redshift z=5.3, is one of the most distant radio-loud objects. Since its radio flux exceeds 100 mJy at a few GHz, it is also one of the most powerful radio-loud sources. We propose that…

宇宙学与河外天体物理 · 物理学 2015-06-11 T. Sbarrato , G. Ghisellini , M. Nardini , G. Tagliaferri , L. Foschini , G. Ghirlanda , F. Tavecchio , J. Greiner , A. Rau , N. Gehrels

We present results of a new, large survey for high-redshift radio-loud quasars, which targets quasars with z>4. The survey is based on the PMN and NVSS radio surveys, optically identified using digitised UKST B, R and I plates. Six new z>4…

天体物理学 · 物理学 2009-11-07 I. M. Hook , R. G. McMahon , P. A. Shaver , I. A. G. Snellen

The radio-loud quasar SDSS J114657.79+403708.6 at a redshift z=5.0 is one of the most distant radio-loud objects. The IR-optical luminosity and spectrum suggest that its black hole has a very large mass: M=(5+-1)x 1e9 Msun. The…

高能天体物理现象 · 物理学 2015-06-18 G. Ghisellini , T. Sbarrato , G. Tagliaferri , L. Foschini , F. Tavecchio , G. Ghirlanda , V. Braito , N. Gehrels

We present the discovery of PSO J191.05696$+$86.43172 (hereafter PSO J191$+$86), a new powerful radio-loud quasar (QSO) in the early Universe (z = 5.32). We discovered it by cross-matching the NRAO VLA Sky Survey (NVSS) radio catalog at 1.4…

星系天体物理 · 物理学 2023-01-25 S. Belladitta , A. Moretti , A. Caccianiga , D. Dallacasa , C. Spingola , M. Pedani , L. P. Cassarà , S. Bisogni

We present a multi-wavelength analysis, from the radio to the X-ray band, of the redshift $z=6.44$ VIK J2318$-$31 radio-loud (RL) quasi stellar object (QSO), one of the most distant currently known in this class. The work is based on newly…

We present optical spectroscopic data for a complete sample of 161 S_5GHz >= 0.2 Jy, flat-spectrum radio sources. The sources were observed as part of a survey for high redshift, radio-loud quasars, and were selected for spectroscopic…

天体物理学 · 物理学 2015-06-24 I. M. Hook , R. G. McMahon , M. J. Irwin , C. Hazard

Radio sources at the highest redshifts can provide unique information on the first massive galaxies and black holes, the densest primordial environments, and the epoch of reionization. The number of astronomical objects identified at z>6…

The radio-loud quasar SDSS J013127.34-032100.1at a redshift z=5.18 is one of the most distant radio-loud objects. The radio to optical flux ratio (i.e. the radio-loudness) of the source is large, making it a promising blazar candidate. Its…

高能天体物理现象 · 物理学 2015-06-23 G. Ghisellini , G. Tagliaferri , T. Sbarrato , N. Gehrels

We present the discovery of PSO J030947.49+271757.31, the radio brightest (23.7 mJy at 1.4 GHz) active galactic nucleus (AGN) at z>6.0. It was selected by cross-matching the NRAO VLA Sky Survey and the Panoramic Survey Telescope and Rapid…

The uncharted territory of the high-redshift ($z\gtrsim3$) Universe holds the key to understand the evolution of quasars. In an attempt to identify the most extreme members of the quasar population, i.e., blazars, we have carried out a…

高能天体物理现象 · 物理学 2020-07-22 Vaidehi S. Paliya , M. Ajello , H. -M. Cao , M. Giroletti , Amanpreet Kaur , Greg Madejski , Benoit Lott , D. Hartmann

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

The detection of high-redshift ($z>$3) blazars enables the study of the evolution of the most luminous relativistic jets over cosmic time. More importantly, high-redshift blazars tend to host massive black holes and can be used to constrain…

高能天体物理现象 · 物理学 2017-04-25 Large Area Telescope Collaboration

Luminous quasars at $z>4$ provide key insights into the early Universe. Their rarity necessitates wide-field multi-band surveys to efficiently separate them from the main astrophysical contaminants (i.e., ultracool dwarfs). To expand the…

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 studied the radio structure of high-redshift (z>3) quasars with VSOP at 1.6 and 5 GHz. These sources are the most distant objects ever observed with Space VLBI, at rest-frame frequencies up to ~25 GHz. Here we give an account of the…

天体物理学 · 物理学 2008-02-01 S. Frey , L. I. Gurvits , A. P. Lobanov , R. T. Schilizzi , Z. Paragi

We present the discovery of the radio-loud quasar PSO J352.4034-15.3373 at z=5.84 pm 0.02. This quasar is the radio brightest source known, by an order of magnitude, at z~6 with a flux density in the range of 8-100 mJy from 3GHz to 230MHz…

Blazars are sources whose jet is pointing to us. Since their jets are relativistic, the flux is greatly amplified in the direction of motion, making blazars the most powerful persistent objects in the Universe. This is true at all…

宇宙学与河外天体物理 · 物理学 2013-02-04 G. Ghisellini

We report the discovery and confirmation of a bright quasi-stellar object (QSO), 2MASS J13260399+7023462, at $z=2.889$. This QSO is the first spectroscopically confirmed candidate from an ongoing search using the combination of Gaia and…

We report on European VLBI Network (EVN) and Very Large Array (VLA) observations of SDSS J0836+0054, the most distant radio-loud quasar known at present z=5.774). The source, with a total flux density of 1.1 mJy, shows a compact structure…

天体物理学 · 物理学 2007-05-23 S. Frey , Z. Paragi , L. Mosoni , L. I. Gurvits

There are about 50 quasars known at redshifts z>5.7 to date. Only three of them are detected in the radio (J0836+0054, z=5.77; J1427+3312, z=6.12; J1429+5447, z=6.21). The highest-redshift quasars are in the forefront of current…

宇宙学与河外天体物理 · 物理学 2011-05-13 S. Frey , Z. Paragi , . L. I. Gurvits , K. É. Gabányi , D. Cseh
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