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We present a Hubble Space Telescope image of the FRII radio galaxy 3C 401, obtained at 1.6 microns with the NICMOS camera in which we identify the infrared counterpart of the brightest region of the radio jet. The jet has a complex radio…

Powerful radio sources and quasars emit relativistic jets of plasma and magnetic fields that travel hundreds of kilo-parsecs, ultimately depositing energy into the intra- or inter-cluster medium. In the rest frame of the jet, the energy…

Extragalactic radio sources with projected linear size larger than one Megaparsec 1 Mpc = 3.09e22 m = 3.3e6 light years) are called Giant Radio Galaxies (GRGs) or quasars (GRQs). Over the past few years our search for such objects by visual…

星系天体物理 · 物理学 2017-11-15 Jonatan Rentería Macario , Heinz Andernach

Context. Blazars are powerful active galactic nuclei (AGNs) radiating prominently in the whole electromagnetic spectrum, from the radio to the X-ray and gamma-ray bands. Their emission is dominated by synchrotron and inverse-Compton…

宇宙学与河外天体物理 · 物理学 2013-04-16 S. Frey , Z. Paragi , K. E. Gabanyi , T. An

We report on the study of an intriguing active galaxy that was selected as a potential multiple supermassive black hole merger in the early-type host SDSS J151709.20+335324.7 (z=0.135). Ground-based SDSS imaging reveals two blue structures…

宇宙学与河外天体物理 · 物理学 2015-05-18 D. J. Rosario , G. A. Shields , G. B. Taylor , S. Salviander , K. L. Smith

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

Spectral analysis of ROSAT PSPC and ASCA archive data and a recent ROSAT HRI observation of the powerful FRII radio galaxy 3C 219 reveal an absorbed point-like source, coincident with the nucleus, and a non-thermal extended component…

天体物理学 · 物理学 2007-05-23 G. Brunetti , A. Comastri , G. Setti , L. Feretti

The properties of radio galaxies and quasars with and without optical or X-ray jets are compared. The majority of jets from which high-frequency emission has been detected so far (13 with optical emission, 11 with X-rays, 13 with both) are…

天体物理学 · 物理学 2008-11-26 S. Jester

We have discovered an obscured active galaxy at redshift z = 1.246 identified with the ROSAT X-ray source RX J1011.2+5545. We report on multiwavelength observations of this source and discuss its X-ray, optical and radio properties. This is…

天体物理学 · 物理学 2007-05-23 X. Barcons , R. Carballo , M. T. Ceballos , R. S. Warwick , J. I. Gonzalez-Serrano

We present the results of Chandra ACIS-S snapshot observations of six radio-loud quasars (RLQs) at z=3.5-4.7. These observations sample luminous RLQs with moderate-to-high radio-loudness (R=200-9600) and aim to connect the X-ray properties…

天体物理学 · 物理学 2008-11-26 L. A. Lopez , W. N. Brandt , C. Vignali , D. P. Schneider , G. Chartas , G. P. Garmire

Using the Spitzer Space Telescope, we have obtained 3.6--24 micron photometry of 38 radio galaxies and 24 quasars from the 3CR catalog at redshift 1<z<2.5. This 178 MHz-selected sample is unbiased with respect to orientation and therefore…

天体物理学 · 物理学 2009-11-13 M. Haas , S. V. P. Willner , F. Heymann , M. L. N. Ashby , G. G. Fazio , B. J. Wilkes , R. Chini , R. Siebenmorgen

Context. NRAO 150 is one of the brightest radio and mm AGN sources on the northern sky. It has been revealed as an interesting source where to study extreme relativistic jet phenomena. However, its cosmological distance has not been…

宇宙学与河外天体物理 · 物理学 2015-05-18 J. A. Acosta-Pulido , I. Agudo , R. Barrena , C. Ramos Almeida , A. Manchado , P. Rodríguez-Gil

We present deep infrared (Ks band) imaging polarimetry and radio (1.4 and 4.8 GHz) polarimetry of the enigmatic transient Swift J164449.3+573451. This source appears to be a short lived jet phenomenon in a galaxy at redshift z = 0.354,…

We present a radio and X-ray study of PKS 1353-341, the brightest cluster galaxy radio source at the center of a recent Chandra-discovered X-ray cluster. Our multi-frequency VLA images reveal an edge-brightened (FR-II), double-lobed…

星系天体物理 · 物理学 2019-05-01 C. C. Cheung , Simona Giacintucci , T. E. Clarke

The results of an X-ray observation of the nearby core-dominated, super- luminal quasar 4C+73.18 (1928+738) with ASCA are reported. Variations of the 1-10keV flux on time-scales of the order of 10 hours were found while the 0.5-1keV flux…

天体物理学 · 物理学 2016-08-30 W. Yuan , W. Brinkmann , M. Gliozzi , Y. Zhao , M. Matsuoka

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

Abridged) In the SDSS, several unusual QSOs have been discovered that have very blue rest-frame UV spectra but no discernible emission lines. Their UV spectra strongly resemble that of the newly discovered quasar PHL 1811 ($z=0.192$; $\rm…

天体物理学 · 物理学 2007-05-23 Karen M. Leighly , Jules P. Halpern , Edward B. Jenkins

We present the radio properties of optically selected quasars with $z\geq3$. The complete sample consists of 102 quasars with a flux density level $S_{1.4}\geq100$ mJy in a declination range -35$^{\circ}$ $\leq$ Dec $\leq$ +49$^{\circ}$.…

We report on the extreme behaviour of the high redshift blazar GB B1428+4217 at z=4.72. A continued programme of radio measurements has revealed an exceptional flare in the lightcurve, with the 15.2 GHz flux density rising by a factor ~3…

天体物理学 · 物理学 2009-09-17 M. A. Worsley , A. C. Fabian , G. G. Pooley , C. J. Chandler

Active galaxies are the most powerful engines in the Universe for converting gravitational energy into radiation, and radio galaxies and radio-loud quasars are highly luminous and can be detected across the Universe. The jets that…

天体物理学 · 物理学 2007-05-23 E. Belsole , D. M. Worrall , M. J. Hardcastle