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相关论文: Exploring the radio-loudness of SDSS quasars with …

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Quasars are objects of high interest in extragalactic astrophysics, cosmology, and astrometry. One of their useful qualities is their potential radio loudness. However, the fraction of radio-loud vs. radio-quiet quasars is subject to…

星系天体物理 · 物理学 2025-08-26 Nestor Arsenov , Sandor Frey , András Kovács , Lyuba Slavcheva-Mihova

We present a detailed analysis of a sample of radio-detected quasars, obtained by matching together objects from the FIRST and 2dF Quasar Redshift Surveys. The dataset consists of 113 sources, spanning a redshift range 0.3 < z < 2.2, with…

天体物理学 · 物理学 2009-11-07 M. Cirasuolo , M. Magliocchetti , A. Celotti , L. Danese

To better constrain the hypotheses proposed to explain why only a few quasars are radio loud (RL), we compare the characteristics of 1958 nearby $(z\le 0.3)$ SDSS quasars, covered by the FIRST and NVSS radio surveys. Only 22\% are RL with…

We examine the distribution of radio emission from ~42,000 quasars from the Sloan Digital Sky Survey, as measured in the LOFAR Two-Metre Sky Survey (LoTSS). We present a model of the radio luminosity distribution of the quasars that assumes…

Radio emission in the brightest radio quasars can be attributed to processes inherent to SMBHs, while the origins of the radio fluxes in quasars without radio detections is still uncertain. We investigate the radio-infrared continuum of…

星系天体物理 · 物理学 2022-07-27 E. Retana-Montenegro

We report on two programs to address differential evolution between the radio-loud and radio-quiet quasar populations at high (z>4) redshift. Both programs entail studying the radio properties of optically-selected quasars. First, we have…

天体物理学 · 物理学 2009-10-31 Daniel Stern , S. G. Djorgovski , R. A. Perley , Reinaldo R. deCarvalho , J. V. Wall

The radio-loud/radio-quiet (RL/RQ) dichotomy in quasars is still an open question. Although it is thought that accretion onto supermassive black holes in the centre the host galaxies of quasars is responsible for some radio continuum…

We present deep radio observations of the most distant complete quasar sample drawn from the Sloan Digital Sky Survey. Combining our new data with those from literature we obtain a sample which is ~100 per cent complete down to S_1.4GHz =…

天体物理学 · 物理学 2009-11-11 M. Cirasuolo , M. Magliocchetti , G. Gentile , A. Celotti , S. Cristiani , L. Danese

Optically luminous quasars at $z > 5$ are important probes of super-massive black hole (SMBH) formation. With new and future radio facilities, the discovery of the brightest low-frequency radio sources in this epoch would be an important…

High redshift quasars ($z>5$) that also shine brightly at radio wavelengths are unique signposts of supermassive black hole activity in the early universe. However, bright radio sources at $z\ge5$ are extremely rare and therefore we have…

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

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 present a study of a sample of 223 radio-loud quasars (up to redshift $<$0.3) in order to investigate their spectral properties. Twenty-six of these radio-loud quasars are identified as Flat Spectrum Radio Quasars (FSRQs) and fifty-four…

高能天体物理现象 · 物理学 2019-10-23 Haritma Gaur , Minfeng Gu , S. Ramya , Hengxiao Guo

Using a sample of more than 6000 quasars from the Sloan digital sky survey (SDSS) we compare the black-hole mass distributions of radio-loud and radio-quiet quasars. Based on the virial black-hole mass estimator the radio-loud quasars…

天体物理学 · 物理学 2009-11-10 R. J. McLure , M. J. Jarvis

We present the study on the X-ray emission for a sample of radio-detected quasars constructed from the cross-matches between SDSS, FIRST catalogs and XMM-Newton archives. A sample of radio-quiet SDSS quasars without FIRST radio detection is…

高能天体物理现象 · 物理学 2021-02-10 Minhua Zhou , Minfeng Gu

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

We investigate the [O II] emission line properties of 18,508 quasars at z<1.6 drawn from the Sloan Digital Sky Survey (SDSS) quasar sample. The quasar sample has been separated into 1,692 radio-loud and 16,816 radio-quiet quasars (RLQs and…

宇宙学与河外天体物理 · 物理学 2015-06-11 E. Kalfountzou , M. J. Jarvis , D. G. Bonfield , M. J. Hardcastle

We present results from uGMRT 685 MHz observations of 87 QSOs belonging to the Palomar Green (PG) quasar sample with $z<0.5$. Radio emission is detected in all sources except for 3 radio-quiet (RQ) sources, viz., PG 0043+039, PG 1121+422,…

星系天体物理 · 物理学 2025-10-06 Sanna Gulati , Silpa Sasikumar , Preeti Kharb , Luis C. Ho , Salmoli Ghosh , Janhavi Baghel

Recent work has shown that it is possible to systematize quasars (QSOs) spectral diversity in 4DE1 parameter space. The spectra contained in most of the surveys have low signal to noise ratio which fed the impression that all QSO\'{s} are…

星系天体物理 · 物理学 2021-07-14 Shimeles Terefe , Ascensión Del Olmo Orozco , Paola Marziani , Mirjana Pović

We search fora dichotomy/bimodality between Radio Loud (RL) and Radio Quiet (RQ) Type 1 Active Galactic Nuclei (AGN). We examine several samples of SDSS QSOs with high S/N optical spectra and matching FIRST/NVSS radio observations. We use…

天体物理学 · 物理学 2009-11-13 Sebastian Zamfir , Jack W. Sulentic , Paola Marziani
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