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相关论文: Kpc-scale Radio Structure in $z\sim0.25$ Radio-Qui…

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We discuss 6 GHz JVLA observations covering a volume-limited sample of 178 low redshift ($0.2 < z < 0.3$) optically selected QSOs. Our 176 radio detections fall into two clear categories: (1) About $20$\% are radio-loud QSOs (RLQs) having…

星系天体物理 · 物理学 2016-11-15 K. I. Kellermann , J. J. Condon , A. E. Kimball , R. A. Perley , Zeljko Ivezic

Although radio-quiet quasars (RQQs) constitute >90% of optically-identified quasar samples their radio properties are only poorly understood. In this paper we present the results of a multi-frequency VLA study of 27 low-redshift RQQs. We…

天体物理学 · 物理学 2015-06-24 M. J. Kukula , J. S. Dunlop , D. H. Hughes , S. Rawlings

We observed 20 Palomar-Green (PG) quasars at low redshift ($z<0.5$) with total flux density > 1 mJy, including 4 radio-loud quasars (RLQs) and 16 radio-quiet quasars (RQQs), using the Very Long Baseline Array (VLBA) at 5 GHz. Ten RQQs are…

星系天体物理 · 物理学 2022-11-01 Ailing Wang , Tao An , Xiaopeng Cheng , Luis C. Ho , Kenneth I. Kellermann , Willem A. Baan , Jun Yang , Yingkang Zhang

We investigate the clustering properties of 45441 radio-quiet quasars (RQQs) and 3493 radio-loud quasars (RLQs) drawn from a joint use of the Sloan Digital Sky Survey (SDSS) and Faint Images of the Radio Sky at 20 cm (FIRST) surveys in the…

星系天体物理 · 物理学 2017-04-12 E. Retana-Montenegro , H. J. A. Röttgering

Although radio-quiet quasars (RQQs), which constitute the majority of optically-identified quasar samples, are by no means radio silent the properties of their radio emission are only poorly understood. We present the results of a…

天体物理学 · 物理学 2009-10-30 Marek J. Kukula , James S. Dunlop , David H. Hughes , Steve Rawlings

Despite decades of study, it remains unclear whether there are distinct radio-loud and radio-quiet populations of quasi-stellar objects (QSOs). Early studies were limited by inhomogeneous QSO samples, inadequate sensitivity to probe the…

宇宙学与河外天体物理 · 物理学 2015-05-28 Amy E. Kimball , Kenneth I. Kellermann , James J. Condon , Zeljko Ivezic , Richard A. Perley

We present Very Large Array observations at 1.4 and 5 GHz of a sample of 16 quasi-stellar objects (QSOs) at z = 1.78 to 2.71. Half of the chosen quasars are bright at mm wavelengths (250 or 350 GHz) while the other half were not detected at…

天体物理学 · 物理学 2008-11-26 A. Petric , C. L. Carilli , F. Bertoldi , A. Beelen , P. Cox , A. Omont

VLA B-configuration snapshots have been obtained at 6cm and 20cm of 43 radio quasars with a range of known galaxy cluster environments. The radio sources are characterised by measures of morphology, flux, and size. These are studied as a…

天体物理学 · 物理学 2009-10-28 J. B. Hutchings , A. C. Gower , S. Ryneveld , A. Dewey

We present the final results from our deep HST imaging study of the hosts of radio-quiet quasars (RQQs), radio-loud quasars (RLQs) and radio galaxies (RGs). We describe new WFPC2 R-band observations for 14 objects and model these images in…

天体物理学 · 物理学 2008-11-26 J. S. Dunlop , R. J. McLure , M. J. Kukula , S. A. Baum , C. P. O'Dea , D. H. Hughes

We have used the Very Long Baseline Array (VLBA) to image five radio-quiet quasars (RQQs) at milliarcsecond resolution, at frequencies between 1.4 and 5 GHz. These quasars have typical total flux densities of a few millijansky at gigahertz…

天体物理学 · 物理学 2009-11-10 James S. Ulvestad , Robert R. J. Antonucci , Richard Barvainis

We present the result of 27 ASCA observations of 26 radio-quiet quasars (RQQs) from the PG survey. All the RQQs were detected except 2 BALQSOs. We find the variability characteristics of the sources to be consistent with Seyf-1s. A powerlaw…

天体物理学 · 物理学 2009-10-31 I. M. George , T. J. Turner , T. Yaqoob , H. Netzer , A. Laor , R. F. Mushotzky , K. Nandra , T. Takahashi

The recent detection of the quasi-stellar object (QSO) VIKING J231818.3$-$311346 (hereafter VIK J2318$-$3113) at redshift $z=6.44$ in the Rapid ASKAP Continuum Survey (RACS) uncovered its radio-loud nature, making it one of the most distant…

Quasars at redshifts $z>6$ are an excellent probe of the formation and evolution of supermassive black holes in the early Universe. The population of radio-luminous quasars is of particular interest, as such quasars could potentially be…

星系天体物理 · 物理学 2024-02-15 Pascal M. Keller , Nithyanandan Thyagarajan , Ajay Kumar , Nissim Kanekar , Gianni Bernardi

The origin of the radio emission in radio-quiet quasars (RQQ) is not established yet. We present new VLBA observations at 1.6 and 4.9 GHz of ten RQQ (nine detected), which together with published earlier observations of eight RQQ (five…

星系天体物理 · 物理学 2023-08-09 Sina Chen , Ari Laor , Ehud Behar , Ranieri D. Baldi , Joseph D. Gelfand

Here we report the X-ray spectral analysis of 5 high-redshift ($z \geq 2$) radio-quiet quasars (RQQs) observed with the ASCA satellite. A simple power law with Galactic absorption model well fits the data. There is no evidence of a…

天体物理学 · 物理学 2007-05-23 C. Vignali , A. Comastri , M. Cappi , G. G. C. Palumbo , M. Matsuoka

This paper presents the first high-resolution and high-sensitivity study of the radio properties of optically selected type~2 quasars. We used the Very Large Array at 8.4 GHz to observe 59 sources drawn from the Sloan Digital Sky Survey…

宇宙学与河外天体物理 · 物理学 2015-05-14 Dharam Vir Lal , Luis C. Ho

We investigate the radio emitting structures of radio-quiet active galactic nuclei with an emphasis on radio-quiet quasars to study their connection to Seyfert galaxies. We present and analyse high-sensitivity VLA radio continuum images of…

天体物理学 · 物理学 2009-11-11 Christian Leipski , Heino Falcke , Nicola Bennert , Susanne Huettemeister , ;

We study the radio properties of moderately obscured quasars over a range of redshifts to understand the role of radio activity in accretion using the Jansky Very Large Array (JVLA) at 6.0GHz and 1.4GHz. Our z~2.5 sample consists of…

We present K-band imaging and photometry of a sample of 52 radio loud quasars (RQs) selected from the B3 survey with flux densities above 0.5 Jy at 408 MHz. The optical completeness of the sample is 90% and the quasars cover the redshift…

天体物理学 · 物理学 2009-10-30 R. Carballo , S. F. Sanchez , J. I. Gonzalez-Serrano , C. R. Benn , M. Vigotti

We present near-infrared H-band imaging of 15 intermediate redshift (0.5<z<1) radio quiet quasars (RQQ) in order to characterize the properties of their host galaxies. We are able to clearly detect the surrounding nebulosity in 12 objects,…

天体物理学 · 物理学 2015-06-24 T. Hyvonen , J. K. Kotilainen , E. Orndahl , R. Falomo , M. Uslenghi
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