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Related papers: Flat-Spectrum Radio Quasars from SDSS DR3 Quasar C…

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We study the broad emission line blazars detected in the gamma-ray band by the Large Area Telescope onboard the Fermi satellite and with the optical spectrum studied by Shaw et al. (2012, 2013). The observed broad line strength provides a…

High Energy Astrophysical Phenomena · Physics 2015-06-23 G. Ghisellini , F. Tavecchio

Based on the classical unification, blazars, namely BL Lacertae objects (BL Lacs) and flat-spectrum radio quasars (FSRQs), are believed to correspond with radio galaxies when observed at small jet viewing angles. In this paper, we aim to…

High Energy Astrophysical Phenomena · Physics 2026-04-01 Xu-Hong Ye , Ranieri D. Baldi , Wen-Xin Yang , Jing-Tian Zhu , Denis Bastieri , Rumen S. Bachev , Anton A. Strigachev , Jun-Hui Fan

We present a detailed analysis of the single-slit optical spectrum of the Flat-Spectrum Radio Quasar (FSRQ) B2 0003+38A, taken by the Echellette Spectrograph and Imager (ESI) on the Keck II telescope. This classical low-redshift FSRQ…

Astrophysics of Galaxies · Physics 2021-06-09 Qinyuan Zhao , Luming Sun , Lu Shen , Guilin Liu , Hongyan Zhou , Tuo Ji

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…

High Energy Astrophysical Phenomena · Physics 2019-10-23 Haritma Gaur , Minfeng Gu , S. Ramya , Hengxiao Guo

Flat-spectrum radio quasars (FSRQs) whose brightness is dominated by a relativistically beamed core, are frequently found in 'blazar state' commonly inferred from a high optical polarization ( > 3%), and/or a large continuum variability.…

Astrophysics of Galaxies · Physics 2022-10-05 Krishan Chand , Gopal-Krishna

A sample of 111 Fermi blazars each with a well-established radio core luminosity, broad-line luminosity, bolometric luminosity and black hole mass has been compiled from the literatures.We present a significant correlation between radio…

High Energy Astrophysical Phenomena · Physics 2015-06-24 Xiaoling Yu , Xiong Zhang , Haojing Zhang , Dingrong Xiong , Bijun Li , Yongjuan Cha , Yongyun Chen , Xia Huang , Yuwei Wang

Our understanding of the unification of jetted AGNs has advanced greatly as the size of extragalactic sources increased. In the present paper, based on the large sample of radio sources, we compiled 680 blazars (279 FSRQs and 401 BL Lacs)…

Astrophysics of Galaxies · Physics 2021-11-17 E. U. Iyida , I. O. Eya , F. C. Odo

A prediction for the energy shift of the synchrotron spectrum of flat-spectrum radio quasars (FSRQs) during high-energy flares is presented. If the $\gamma$-ray emission of FSRQs is produced by Comptonization of external radiation, then the…

Astrophysics · Physics 2009-10-31 M. Boettcher

We present results based on the first 20 Chandra images obtained in a survey of jets in radio selected flat-spectrum quasars (FSRQs), along with new sub-arcsecond radio maps and optical images. We discover jet X-ray flux in 12 sources…

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,…

Astrophysics of Galaxies · Physics 2025-10-06 Sanna Gulati , Silpa Sasikumar , Preeti Kharb , Luis C. Ho , Salmoli Ghosh , Janhavi Baghel

We propose and test a fairly simple idea that could account for the blazar sequence: all jets are launched with similar energy per baryon, independently of their power. For instance, flat-spectrum radio quasars (FSRQs), the most powerful…

High Energy Astrophysical Phenomena · Physics 2021-01-13 Jesús M. Rueda-Becerril , Amanda O. Harrison , Dimitrios Giannios

We revisit the blazar sequence exploiting the complete, flux limited sample of blazars with known redshift detected by the Fermi satellite after 4 years of operations (the 3LAC sample). We divide the sources into gamma-ray luminosity bins,…

High Energy Astrophysical Phenomena · Physics 2017-05-31 G. Ghisellini , C. Righi , L. Costamante , F. Tavecchio

We present multiwavelength data for twelve blazars observed from 2008-2010 as part of an ongoing optical-infrared photometric monitoring project. Sources were selected to be bright, southern (dec < 20 deg) blazars observed by the Fermi…

High Energy Astrophysical Phenomena · Physics 2015-06-03 E. W. Bonning , C. M. Urry , C. Bailyn , M. Buxton , R. Chatterjee , P. Coppi , G. Fossati , J. Isler , L. Maraschi

This work studies the relationship between accretion-disk size and quasar properties, using a sample of 95 quasars from the SDSS-RM project with measured lags between the $g$ and $i$ photometric bands. Our sample includes disk lags that are…

The mechanisms responsible for the production of relativistic jets from supermassive black holes (SMBHs) accreting at near-Eddington rates are not well-understood. Simple theoretical expectations indicate that SMBHs in quasars accrete via…

High Energy Astrophysical Phenomena · Physics 2020-05-13 Gustavo Soares , Rodrigo Nemmen

ROSAT observations of a large sample of bright gamma-ray (E > 100 MeV) blazars are presented. Results of a detailed spectral analysis in the soft $\sim$ 0.1-2.0 keV energy range are discussed in relation to the overall energy distribution…

Astrophysics · Physics 2016-08-30 A. Comastri , G. Fossati , G. Ghisellini , S. Molendi

We present statistical analyses of a large homogenous data sample of Fermi-detected blazars thoroughly studied in order to reassess the relationship between flat-spectrum radio quasars (FSRQs) and subclasses of BL Lacertae objects (BL Lacs)…

High Energy Astrophysical Phenomena · Physics 2021-08-18 E. U. Iyida , F. C. Odo , A. E. Chukwude , A. A. Ubachukwu

We present radio spectra spanning $0.1 - 10$ GHz for the sample of heavily obscured luminous quasars with extremely red mid-infrared-optical colors and compact radio emission. The spectra are constructed from targeted 10 GHz observations…

Extended extragalactic radio sources have traditionally been classified into FR I and II types, based on the ratio r of the separation S between the brightest regions on either sides of the host galaxy and the total size T of the radio…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Yen-Ting Lin , Yue Shen , Michael Strauss , Gordon Richards , Ragnhild Lunnan

Using three complete, radio flux limited, blazar samples we compare the LogN-LogS and the preliminary radio luminosity function of the general population of BL Lacs to those of the subclass of high energy synchrotron peaked (HBL) BL Lacs.…

Astrophysics · Physics 2007-05-23 P. Giommi , P. Padovani , M. Perri , H. Landt , E. Perlman
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