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相关论文: 4C 02.27: what is inside a double-double radio qua…

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The radio source J0028+0035 is a recently discovered double--double radio galaxy at redshift z=0.398. Its relic outer lobes are separated by about 3' in the sky, corresponding to ~1 Mpc projected linear size. Inside this large-scale…

星系天体物理 · 物理学 2025-01-27 S. Frey , A. Marecki , K. É. Gabányi , M. Jamrozy

Striking examples of episodic activity in active galactic nuclei are the double-double radio galaxies (DDRGs) with two pairs of oppositely-directed radio lobes from two different cycles of activity. Although there are over about a dozen…

宇宙学与河外天体物理 · 物理学 2015-05-13 M. Jamrozy , D. J. Saikia , C. Konar

Context: The highest redshift quasars at z>~6 receive considerable attention since they provide strong constraints on the growth of the earliest supermassive black holes. They also probe the epoch of reionisation and serve as "lighthouses"…

天体物理学 · 物理学 2008-06-10 S. Frey , L. I. Gurvits , Z. Paragi , K. E. Gabanyi

Context: Until now, there have only been seven quasars at z>4.5 whose the high-resolution radio structure had been studied in detail with Very Long Baseline Interferometry (VLBI) imaging. Aims: We almost double the number of VLBI-imaged…

宇宙学与河外天体物理 · 物理学 2010-11-30 S. Frey , Z. Paragi , L. I. Gurvits , D. Cseh , K. E. Gabanyi

Context. Radio-loud active galactic nuclei in the early Universe are rare. The quasars J0906+6930 at redshift z=5.47 and J2102+6015 at z=4.57 stand out from the known sample with their compact emission on milliarcsecond (mas) angular scale…

星系天体物理 · 物理学 2018-10-17 S. Frey , O. Titov , A. E. Melnikov , P. de Vicente , F. Shu

We show an archival 1.4-GHz Very Large Array (VLA) image of the core-dominated triple (CDT) radio source J1628+3906, along with a recent high-resolution 5-GHz Very Long Baseline Interferometry (VLBI) image of its core. This core is resolved…

天体物理学 · 物理学 2009-04-14 D. Cseh , A. Fuhl , S. Frey

Giant double-lobed radio source 4C34.47 displays a straight one-sided jet, measuring a record length of 380kpc, in its double-lobed radio structure. Assuming an intrinsically symmetric two-sided jet structure the radio source jet axis must…

星系天体物理 · 物理学 2015-05-19 S. Hocuk , P. D. Barthel

Many low-luminosity active galactic nuclei (AGNs) contain a compact radio core which can be observed with high angular resolution using very long baseline interferometry (VLBI). Combining arcsec-scale structural information with…

星系天体物理 · 物理学 2020-04-06 Máté Krezinger , Sándor Frey , Zsolt Paragi , Roger Deane

We present a study of the peculiar radio galaxy B 1834+620. It is characterised by the presence of a 420-kpc large edge-brightened radio source which is situated within, and well aligned with, a larger (1.66 Mpc) radio source. Both sources…

天体物理学 · 物理学 2009-10-31 Arno P. Schoenmakers , A. G. de Bruyn , H. J. A. Rottgering , H. van der Laan

We present radio, optical, near-infrared and spectroscopic observations of the source B0827+525. We consider this source as the best candidate from the Cosmic Lens All-Sky Survey (CLASS) for a `dark lens' system or binary radio-loud quasar.…

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

New Chandra observations of the giant (0.5 Mpc) radio galaxy 4C23.56 at z = 2.5 show X-rays in a linear structure aligned with its radio emission, but anti-correlated with the detailed radio structure. Consistent with the powerful, high-z…

宇宙学与河外天体物理 · 物理学 2015-05-19 Katherine Blundell , Andy Fabian

We report the discovery of two radio-loud quasars with redshifts greater than four; GB1428+4217 with z=4.72 and GB1713+2148 with z=4.01. This doubles the number of published radio-selected quasars with z > 4, bringing the total to 4.…

天体物理学 · 物理学 2020-11-25 I. M. Hook , R. G. McMahon

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

The powerful high-redshift quasar J2102+6015 (at z=4.575) may provide useful information for studying supermassive black hole growth, galaxy evolution and feedback in the early Universe. The source has so far been imaged with very long…

星系天体物理 · 物理学 2023-03-20 S. Frey , T. An , K. Gabányi , L. Gurvits , M. Krezinger , A. Melnikov , P. Mohan , Z. Paragi , K. Perger , F. Shu , O. Titov , P. de Vicente , Y. Zhang

The so-called double-double structure in radio sources is the most conspicuous signature of their restarted activity. Observations indicate that in the majority of double-double radio sources (DDRS), the span of the radio lobes is larger…

宇宙学与河外天体物理 · 物理学 2009-10-28 Andrzej Marecki , Marek Szablewski

Context: There are about 60 quasars known at redshifts z>5.7 to date. Only three of them are detected in the radio above 1 mJy flux density at 1.4 GHz frequency. Among them, J1429+5447 (z=6.21) is the highest-redshift radio quasar known at…

宇宙学与河外天体物理 · 物理学 2013-04-16 S. Frey , Z. Paragi , L. I. Gurvits , K. É. Gabányi , D. Cseh

We report the discovery of a double-double radio source (DDRS) J0028+0035. We observed it with LOFAR, GMRT, and the VLA. By combining our observational data with those from the literature, we gathered an appreciable set of radio flux…

星系天体物理 · 物理学 2020-12-29 A. Marecki , M. Jamrozy , J. Machalski , U. Pajdosz-Smierciak

We present new X-ray and optical spectroscopy of a Type 2 quasar candidate selected from a follow-up program of hard, optically-dim, serendipitous Chandra sources. The source is confirmed to be a Type 2 quasar at z=0.536 with an intrinsic…

天体物理学 · 物理学 2009-09-29 P. Gandhi , A. C. Fabian , C. S. Crawford

We have combined a sample of 44984 quasars, selected from the Sloan Digital Sky Survey (SDSS) Data Release 3, with the FIRST radio survey. Using a novel technique where the optical quasar position is matched to the complete radio…

天体物理学 · 物理学 2009-11-11 W. H. de Vries , R. H. Becker , R. L. White
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