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Related papers: The M_BH - L_rad Relation for Flat-Spectrum Quasar…

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We perform an analysis of the properties of radio-loud (RL) and radio-quiet (RQ) quasars with MgII broad emission line (i-band magnitude $\leq 19.1$ and z $\leq 1.9$), selected from the parent sample of SDSS DR7 catalogue. For sources with…

Astrophysics of Galaxies · Physics 2021-10-22 Avinanda Chakraborty , Anirban Bhattacharjee , Suchetana Chatterjee

We use recent progress in simulating the production of magnetohydrodynamic jets around black holes to derive the cosmic spin history of the most massive black holes, with masses >~10^8 Msol. Assuming the jet efficiency depends on spin a, we…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Alejo Martinez-Sansigre , Steve Rawlings

This paper presents XMM-Newton and Chandra X-ray spectroscopy of ten flat-spectrum radio quasars (FSRQ) which are candidates to have an X-ray spectrum dominated by jet synchrotron emission. In all these FSRQ, which are less strongly…

Astrophysics · Physics 2010-11-11 Hermine Landt , Paolo Padovani , Paolo Giommi , Matteo Perri , Chi C. Cheung

There is general consensus that active galactic nuclei (AGNs) derive their radiating power from a supermassive black hole (SMBH) that accretes matter. Yet, their precise powering mechanisms and the resulting growth of the SMBH are poorly…

Astrophysics of Galaxies · Physics 2025-05-21 Jose Maria Sanchez Zaballa , Eugenio Bottacini , Andrea Tramacere

This paper presents new optical and near-UV spectra of 11 extremely powerful jetted quasars, with radio to optical flux density ratio $>$ 10$^3$, that concomitantly cover the low-ionization emission of \mgii\ and \hb\ as well as the \feii\…

The radio quasar NVSS J141922$-$083830 (J1419$-$0838) was initially classified as an uncategorised blazar-type object, following its detection in the $\gamma$-ray band with the Fermi space telescope. Later, using multi-waveband observations…

High Energy Astrophysical Phenomena · Physics 2023-03-28 Krisztina Perger , Sándor Frey , Krisztina Éva Gabányi

Flat Spectrum Radio Quasars (FSRQ) are the most powerful blazars in the gamma-ray band. Although they are supposed to be good candidates in producing high energy neutrinos, no secure detection of FSRQs has been obtained up to now, except…

High Energy Astrophysical Phenomena · Physics 2020-10-14 C. Righi , A. Palladino , F. Tavecchio , F. Vissani

We are conducting an X-ray survey of flat spectrum radio quasars (FSRQs) with extended radio structures. We summarize our results from the first stage of our survey, then we present findings from its continuation. We have discovered jet…

Whether the mass of supermassive black hole ($M_\mathrm{BH}$) is directly linked to the quasar radio luminosity remains a long-debated issue, and understanding the role of $M_\mathrm{BH}$ in the evolution of quasars is pivotal to unveiling…

In this Letter, the properties of the extended radio emission form SDSS DR7 quasars with $0.4<z<0.8$ is studied. This low redshift sample is useful since any corresponding FIRST radio observations are sensitive enough to detect extended…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Brian Punsly , Shaohua Zhang

The relationship between the black hole mass and velocity dispersion indicated with [O III] line width is investigated for a sample of 87 flat-spectrum radio quasars (FSRQs) selected from SDSS DR3 quasar catalogue. We found the M_bh -…

Astrophysics of Galaxies · Physics 2015-05-13 Minfeng Gu , Zhaoyu Chen , Xinwu Cao

We propose a scenario where blazars are classified as flat-spectrum radio quasars (FSRQs), BL Lacs, low synchrotron, or high synchrotron peaked objects according to a varying mix of the Doppler boosted radiation from the jet, the emission…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 P. Giommi , P. Padovani , G. Polenta , S. Turriziani , V. D'Elia , S. Piranomonte

Blazars are a sub-class of quasars with Doppler boosted jets oriented close to the line of sight, and thus efficient probes of supermassive black hole growth and their environment, especially at high redshifts. Here we report on Very Long…

The central black-hole masses of a sample of 30 luminous quasars are estimated using H-beta FWHM measurements from a combination of new and previously-published nuclear spectra. The quasar black-hole mass estimates are combined with…

Astrophysics · Physics 2009-10-31 R. J. McLure , J. S. Dunlop

The very high-energy (VHE; $>$100 GeV) radiation carries the signatures of the matter-energy interaction in some of the most extreme astrophysical environments. Considering broad emission line blazars, i.e., flat spectrum radio quasars…

High Energy Astrophysical Phenomena · Physics 2025-08-26 Vaidehi S. Paliya , Markus Bottcher , Kiran Wani , P. N. Naseef Mohammed , C. S. Stalin , S. Sahayanathan , D. J. Saikia , S. Muneer

We study the effect of variable jet bulk Lorentz factors, i.e., either jet acceleration or deceleration, on partially synchrotron self-absorbed radio spectra from cores of radio-loud active galactic nuclei and black-hole binaries in the…

High Energy Astrophysical Phenomena · Physics 2019-08-21 Andrzej A. Zdziarski

We present the results of a high resolution (0.27 arcsec/px) near-infrared H band (1.65 micron) imaging survey of a complete sample of 20 flat spectrum radio quasars (FSRQ) extracted from the 2Jy catalogue of radio sources. The observed…

Astrophysics · Physics 2016-08-30 J. K. Kotilainen , R. Falomo , R. Scarpa

We obtained SDSS spectra for a set of 37 radio-quiet quasars (RQQSOs) that had been previously examined for rapid small scale optical variations, or microvariability. Their H-beta and Mg II emission lines were carefully fit to determine…

Cosmology and Nongalactic Astrophysics · Physics 2010-02-04 Hum Chand , Paul J. Wiita , Alok C. Gupta

The jet formation is thought to be closely connected with the mass of central supermassive black hole in Active Galactic Nuclei. The radio luminosity commonly used in investigating this issue is merely an indirect measure of the energy…

Astrophysics · Physics 2008-11-26 Yi Liu , Dong Rong Jiang , Min Feng Gu

We have quantified the galaxy environments around a sample of 0.5 < z < 0.8 radio-quiet quasars using the amplitude of the spatial galaxy--quasar correlation function, B_gq. The quasars exist in a wide variety of environments, some sources…

Astrophysics · Physics 2009-10-31 M. Wold , M. Lacy , P. B. Lilje , S. Serjeant