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Related papers: Detecting Relativistic X-ray Jets in High-Redshift…

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Up to now, jet kinematic studies of radio quasars have barely reached beyond the redshift range at $z>3.5$. This significantly limits our knowledge of high-redshift jets, which can provide key information for understanding the jet nature…

High Energy Astrophysical Phenomena · Physics 2023-03-20 Yingkang Zhang , Tao An , Sandor Frey , Krisztina Eva Gabanyi , Yulia Sotnikova

We report spectral, imaging, and variability results from four new XMM-Newton observations and two new Chandra observations of high-redshift (z > 4) radio-loud quasars (RLQs). Our targets span lower, and more representative, values of radio…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 C. Saez , W. N. Brandt , O. Shemmer , L. Chomiuk , L. A. Lopez , H. L. Marshall , B. P. Miller , C. Vignali

We report on the X-ray emission from the radio jet of 3C 17 from Chandra observations and compare the X-ray emission with radio maps from the VLA archive and with the optical-IR archival images from the Hubble Space Telescope. X-ray…

High Energy Astrophysical Phenomena · Physics 2011-02-11 F. Massaro , D. E. Harris , M. Chiaberge , P. Grandi , F. D. Macchetto , S. A. Baum , C. P. O'Dea , A. Capetti

Much effort has been done in order to better understand the active galactic nuclei mechanisms behind the relativistic jets observed in radio-loud sources. These phenomena are commonly seen in luminous objects with intermediate/high redshift…

Astrophysics of Galaxies · Physics 2022-05-31 A. Deconto-Machado , A. del Olmo Orozco , P. Marziani

The Chandra X-ray observatory has proven to be a vital tool for studying high-energy emission processes in jets associated with Active Galactic Nuclei (AGN).We have compiled a sample of 27 AGN selected from the radio flux-limited MOJAVE…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Brandon Hogan , Matthew Lister , Preeti Kharb , Herman Marshall , Nathan Cooper

The recent discovery of an X-ray jet in the z=4.3 quasar GB 1508+5714 by Yuan et al. (astro-ph/0309318) and Siemiginowska et al. (astro-ph/0310241) prompted a search for its radio counterpart. Here, we report the successful discovery of…

Astrophysics · Physics 2009-11-10 C. C. Cheung

The X-ray emission mechanism of powerful extragalactic jets, which has important implications for their environmental impact, is poorly understood. The X-ray/radio positional offsets in individual features of jets provide important clues.…

High Energy Astrophysical Phenomena · Physics 2023-03-01 Karthik Reddy , Markos Georganopoulos , Eileen T. Meyer , Mary Keenan , Kassidy E. Kollman

The quasar PKS 0637-753, the first celestial X-ray target of the Chandra X-ray Observatory, has revealed asymmetric X-ray structure extending from 3 to 12 arcsec west of the quasar, coincident with the inner portion of the jet previously…

Quasars with flat radio spectra and one-sided, arc-second scale, ~100 mJy GHz radio jets are found to have similar scale X-ray jets in about 60% of such objects, even in short 5 to 10 ks Chandra observations. Jets emit in the GHz band via…

High Energy Astrophysical Phenomena · Physics 2020-03-04 Daniel A. Schwartz

We present the results from an X-ray and optical survey of a sample of 17 radio jets in AGN performed with Chandra and HST. The sample was selected from the radio and is unbiased toward detection at shorter wavelengths, but preferentially…

We present {\it Chandra} X-ray Observatory observations of Giga-Hertz Peaked Spectrum (GPS) and Compact Steep Spectrum (CSS) radio sources. The {\it Chandra} sample contains 13 quasars and 3 galaxies with measured 2-10 keV X-ray luminosity…

We discuss a probe of the contribution of wind-related shocks to the radio emission in otherwise radio-quiet quasars. Given 1) the non-linear correlation between UV and X-ray luminosity in quasars, 2) that such correlation leads to higher…

We present a ~100 ksec Chandra X-ray observation and new VLA radio data of the large scale, 300 kpc long X-ray jet in PKS1127-145, a radio loud quasar at redshift z=1.18. With this deep X-ray observation we now clearly discern the complex…

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

We present arc-second-resolution data in the radio, IR, optical and X-ray for 4C+19.44 (=PKS 1354+195), the longest and straightest quasar jet with deep X-ray observations. We report results from radio images with half to one arc-second…

The Chandra Multiwavelength Project (ChaMP) has discovered a jet-like structure associated with a newly recognized QSO at redshift z=1.866. The system was 9.4 arcmin off-axis during an observation of 3C 207. Although significantly distorted…

The X-ray spectrum of the Galactic microquasar SS 433 contains a rich set of emission lines of highly ionized atoms of heavy elements whose significant Doppler shift leaves no doubt that they are produced in collimated relativistic jets of…

High Energy Astrophysical Phenomena · Physics 2020-05-27 P. Medvedev , I. Khabibullin , S. Sazonov

We report the discovery of a one-sided 3.6" (24 kpc, projected) long jet in the high-redshift, z=4.72, quasar GB 1428+4217 in new Chandra X-ray and VLA radio observations. This is the highest redshift kiloparsec-scale X-ray/radio jet known.…

High Energy Astrophysical Phenomena · Physics 2015-06-11 C. C. Cheung , L. Stawarz , A. Siemiginowska , D. Gobeille , J. F. C. Wardle , D. E. Harris , D. A. Schwartz

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…

We present Chandra X-ray (0.2-8 keV) and Very Large Array radio (15 and 5 GHz) images of the $\gamma$-ray bright, superluminal quasar 0827+243. The X-ray jet bends sharply--by ~90 deg., presumably amplified by projection effects--5'' from…

Astrophysics · Physics 2009-11-10 Svetlana Jorstad , Alan Marscher