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Despite the fact that kpc-scale inverse-Compton (iC) scattering of cosmic microwave background (CMB) photons into the X-ray band is mandated, proof of detection in resolved quasar jets is often insecure. High redshift provides favourable…

High Energy Astrophysical Phenomena · Physics 2020-07-15 D. M. Worrall , M. Birkinshaw , H. L. Marshall , D. A. Schwartz , A. Siemiginowska , J. F. C. Wardle

PKS J2310-437 is an AGN with bright X-ray emission relative to its weak radio emission and optical continuum. It is believed that its jet lies far enough from the line of sight that it is not highly relativistically beamed. It thus provides…

High Energy Astrophysical Phenomena · Physics 2009-11-16 A. F. Bliss , D. M. Worrall , M. Birkinshaw , S. S. Murray , H. Tananbaum

We present the results from the Suzaku X-ray observations of five flat-spectrum radio quasars (FSRQs), namely PKS0208-512, Q0827+243, PKS1127-145, PKS1510-089 and 3C 454.3. All these sources were additionally monitored simultaneously or…

High Energy Astrophysical Phenomena · Physics 2015-05-18 LAT Collaboration , A. A. Abdo , F. Tavecchio , M. Sikora , P. Schady , P. Roming , M. M. Chester , L. Maraschi

We explore the radio properties of powerful (rest-frame luminosity $\gtrsim10^{28}$ W Hz$^{-1}$ at 500 MHz) high-redshift (z > 3.5) quasars. The aim of this study is to gain a better understanding of radio-loud sources at the epoch when…

Astrophysics of Galaxies · Physics 2024-07-02 Alessandro Capetti , Barbara Balmaverde

We report on new multi-frequency Very Large Array (VLA) radio observations and Chandra X-ray observations of a radio-loud quasar with a ~300 kpc long jet, PKS 1127-145, during a flaring event detected in $\gamma$-rays by the Fermi Large…

High Energy Astrophysical Phenomena · Physics 2024-07-24 M. Orienti , A. Siemiginowska , F. D'Ammando , G. Migliori

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…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Dharam Vir Lal , Luis C. Ho

We report on two surveys of radio-weak AGN to look for radio variability. We find significant variability with an RMS of 10-20% on a timescale of months in radio-quiet and radio-intermediate quasars. This exceeds the variability of radio…

Astrophysics · Physics 2007-05-23 Heino Falcke , Joseph Lehar , Richard Barvainis , Neil M. Nagar , Andrew S. Wilson

PKS 2155-304 is one of the brightest BL Lac object in the sky and a very well studied target from radio to TeV bands. We report on high-resolution (~ 0.12 arcsec) direct imaging of the field of PKS 2155-304 using adaptive optics near-IR…

We have measured the mid-infrared radiation from an orientation-unbiased sample of powerful 3C RR galaxies and quasars using the IRS and MIPS instruments aboard the Spitzer Space Telescope. We fit the Spitzer data as well as other…

Astrophysics · Physics 2007-07-30 Kieran Cleary , Charles R. Lawrence , Jason A. Marshall , Lei Hao , David Meier

We present multiwaveband observations of a well selected sample of 28 quasars and two radio galaxies with flat radio spectra and strong millimeter wave emission (referred to here as FSRQ's). The observations include multifrequency VLBI…

Some quasars show Doppler shifted broad emission line peaks. I give new statistics of the occurrence of these peaks and show that, while the most spectacular cases are in quasars with strong radio jets inclined to the line of sight, they…

Astrophysics · Physics 2015-06-24 C. M. Gaskell

We present optical spectroscopy of 62 objects selected from several samples of ultra steep spectrum (USS) radio sources. 46 of these are from our primary catalog, consisting of 669 sources with radio spectral indices alpha < -1.30 (S_nu ~…

Context. Radio-loud AGNs with powerful relativistic jets are thought to be associated with rapidly spinning black holes (BHs). BH spin-up may result from a number of processes, including accretion of matter onto the BH itself, and…

We present the results from 685 MHz observations with the upgraded Giant Metrewave Radio Telescope (uGMRT) of 22 quasars belonging to the Palomar-Green (PG) quasar sample. Only four sources reveal extended radio structures on $\sim$10-30…

Astrophysics of Galaxies · Physics 2020-12-22 Silpa S. , P. Kharb , L. C. Ho , C. H. Ishwara-Chandra , M. E. Jarvis , C. Harrison

We present a multi-wavelength study of IC 1531 (z=0.02564), an extragalactic radio source associated with the $\gamma$-ray object 3FGL J0009.9-3206 and classified as a blazar of uncertain type in the Third Fermi Large Area Telescope AGN…

High Energy Astrophysical Phenomena · Physics 2018-10-17 T. Bassi , G. Migliori , P. Grandi , C. Vignali , M. A. Pérez-Torres , R. D. Baldi , E. Torresi , A. Siemiginowska , C. Stanghellini

We have discovered a number of relatively strong radio sources in the field-of-view of SDSS galaxy clusters which present no optical counterparts down to the magnitude limits of the SDSS. The optically faint radio sources appear as…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Mercedes E. Filho , Jarle Brinchmann , Catarina Lobo , Sonia Antón

The Swift Burst Alert Telescope (BAT) is discovering interesting new objects while monitoring the sky in the 14-195 keV band. Here we present the X-ray properties and spectral energy distributions for two unusual AGN sources. Both NVSS…

High Energy Astrophysical Phenomena · Physics 2015-06-04 J. Drew Hogg , Lisa M. Winter , Richard Mushotzky , Christopher Reynolds , Margaret Trippe

PKS 0521-36 is an Active Galactic Nucleus (AGN) with uncertain classification. We investigate the properties of this source from radio to gamma rays. The broad emission lines in the optical and UV bands and steep radio spectrum indicate a…

High Energy Astrophysical Phenomena · Physics 2015-11-11 F. D'Ammando , M. Orienti , F. Tavecchio , G. Ghisellini , E. Torresi , M. Giroletti , C. M. Raiteri , P. Grandi , M. Aller , H. Aller , M. A. Gurwell , G. Malaguti , E. Pian , G. Tosti

Quasar feedback is a key ingredient in shaping galaxy evolution. A rare population of extremely red quasars (ERQs) at $z=2-3$ are often associated with high-velocity [O III]$\lambda5008$ outflows and may represent sites of strong feedback.…

Astrophysics of Galaxies · Physics 2024-08-13 Yilun Ma , Andy Goulding , Jenny E. Greene , Nadia L. Zakamska , Dominika Wylezalek , Yan-Fei Jiang

We present a $z = 0.94$ quasar, SDSS J004846.45-004611.9, discovered in the SDSS-III BOSS survey. A visual analysis of this spectrum reveals highly broadened and blueshifted narrow emission lines, in particular [Ne~V]$\lambda3426$ and…