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相关论文: SDSS J102623.61+254259.5: the second most distant …

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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

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 report the discovery of a radio-loud flat-spectrum QSO at z=5.47 with properties similar to those of the EGRET gamma-ray blazars. This source is the brightest radio QSO at z>5, with a pc-scale radio jet and a black hole mass estimate…

天体物理学 · 物理学 2009-11-10 Roger W. Romani , David Sowards-Emmerd , Lincoln Greenhill , Peter Michelson

We have selected SDSS J222032.50+002537.5 and SDSS J142048.01+120545.9 as best blazar candidates out of a complete sample of extremely radio-loud quasars at z>4, with highly massive black holes. We observed them and a third serendipitous…

高能天体物理现象 · 物理学 2015-06-23 T. Sbarrato , G. Ghisellini , G. Tagliaferri , L. Foschini , M. Nardini , F. Tavecchio , N. Gehrels

Only very few z>5 quasars discovered to date are radio-loud, with a radio-to-optical flux ratio (radio-loudness parameter) higher than 10. Here we report the discovery of an optically luminous radio-loud quasar, SDSS J013127.34-032100.1…

Based on its broad-band spectral energy distribution, and the X-ray spectrum in particular, the radio-loud active galactic nucleus (AGN) SDSS J102623.61+254259.5 (J1026+2542) has recently been classified as a blazar. The extremely high…

宇宙学与河外天体物理 · 物理学 2013-04-16 S. Frey , J. O. Fogasy , Z. Paragi , L. I. Gurvits

We observed SDSS J0836+0054, the most distant radio-loud quasar known at present (z=5.774) with the European Very Long Baseline Interferometry (VLBI) Network at the 5 GHz frequency on 2003 November 4. The source is compact at the…

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

Few high-redshift, radio-loud quasars are known to date. The extremely luminous, radio-bright quasar, SDSS J013127.34-032100.1 was recently discovered at a redshift of $z=5.18$. We observed the source with high resolution very long baseline…

高能天体物理现象 · 物理学 2015-11-23 K. E. Gabanyi , D. Cseh , S. Frey , Z. Paragi , L. I. Gurvits , T. An , Y. K. Zhang

We investigate the relative occurrence of radio--loud and radio-quiet quasars in the first billion years of the Universe, powered by black holes heavier than one billion solar masses. We consider the sample of high-redshfit blazars detected…

高能天体物理现象 · 物理学 2015-05-27 Marta Volonteri , Francesco Haardt , Gabriele Ghisellini , Roberto Della Ceca

We report the 888 MHz radio detection in the Rapid ASKAP Continuum Survey (RACS) of VIK J2318$-$3113, a $z$=6.44 quasar. Its radio luminosity (1.2 $\times 10^{26}$ W Hz$^{-1}$ at 5 GHz) compared to the optical luminosity (1.8 $\times…

星系天体物理 · 物理学 2021-03-24 L. Ighina , S. Belladitta , A. Caccianiga , J. W. Broderick , G. Drouart , A. Moretti , N. Seymour

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

We present near-infrared H and K-band spectra of the z=6.41 quasar SDSS J114816.64+525150.3. The spectrum reveals a broad MgII 2799 emission line with a full-width half-maximium of 6000 km/s. From the peak wavelength of this emission line…

天体物理学 · 物理学 2009-11-07 Chris J. Willott , Ross J. McLure , Matt J. Jarvis

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 extremely high redshift (z=5.3) radio source SDSS J102623.61+254259.5 (J1026+2542) is among the most distant and most luminous radio-loud active galactic nuclei (AGN) known to date. Its one-sided radio jet structure on milli-arcsecond…

星系天体物理 · 物理学 2014-12-03 S. Frey , Z. Paragi , J. O. Fogasy , L. I. Gurvits

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…

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…

Jets may have contributed to promoting the growth of seed black holes in the early Universe, and thus observations of radio-loud high-redshift quasars are crucial to understanding the growth and evolution of the early supermassive black…

We report Very Long Baseline Array (VLBA) observations of the 1.5 GHz radio continuum emission of the {\it z=6.326} quasar SDSS J010013.02+280225.8 (hereafter J0100+2802). J0100+2802 is, by far the most optically luminous, and radio-quiet…

We report the discovery of X-ray emission from CFHQS J142952+544717, the most distant known radio-loud quasar at z=6.18, on Dec. 10--11, 2019 with the eROSITA telescope on board the SRG satellite during its ongoing all-sky survey. The…

高能天体物理现象 · 物理学 2020-08-12 P. Medvedev , S. Sazonov , M. Gilfanov , R. Burenin , G. Khorunzhev , A. Meshcheryakov , R. Sunyaev , I. Bikmaev , E. Irtuganov

So far, roughly 40 quasars with redshifts greater than z=6 have been discovered. Each quasar contains a black hole with a mass of about one billion solar masses ($10^9 M_\odot$). The existence of such black holes when the Universe was less…

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