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Related papers: A Chandra Search for X-Ray Jets in Redshift 6 Quas…

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We have discovered an X-ray jet with Chandra imaging of the z=1.187 radio-loud quasar PKS1127-145. In this paper we present the Chandra X-ray data, follow-up VLA observations, and optical imaging using the HST WFPC2. The X-ray jet contains…

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

With its exquisite spatial resolution of better than 0.5 arcsecond, the Chandra observatory is uniquely capable of resolving and studying the spatial structure of extragalactic X-ray jets on scales of a few to a few hundred kilo-parsec. Our…

We present results from deep (70 ks) Chandra ACIS observations and Hubble Space Telescope ACS F475W observations of two highly optically polarized quasars belonging to the MOJAVE blazar sample, viz., PKS B0106+013 and 1641+399 (3C345).…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Preeti Kharb , Matthew Lister , Herman Marshall , Brandon Hogan

The jet of the quasar 3C273 is observed at different spectral bands. This jet has a knot structure. Jet radiation in radio and optical bands are connected with synchrotron mechanism, while the emission mechanism producing the X-rays is…

Astrophysics · Physics 2007-12-11 E. Yu. Bannikova , M. S. Mykhailova

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 jet in 3C273 is a high-power quasar jet with radio, optical and X-ray emission whose size and brightness allow a detailed study of the emission processes acting in it. We present deep Chandra observations of this jet and analyse the…

Astrophysics · Physics 2008-11-26 S. Jester , D. E. Harris , H. L. Marshall , K. Meisenheimer

The core-dominated radio-loud quasar PKS 0637-752 (z = 0.654) was the first celestial object observed with the Chandra X-ray Observatory, offering the early surprise of the detection of a remarkable X-ray jet. Several observations with a…

We discuss the physical properties of four quasar jets imaged with the Chandra X-ray Observatory in the course of a survey for X-ray emission from radio jets. These objects have sufficient counts to study their spatially resolved…

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

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

We report results from Chandra observations of the X-ray jet of 3C~273 during the calibration phase in 2000 January. The zeroeth-order images and spectra from two 40-ks exposures with the HETG and LETG+ACIS-S show a complex X-ray structure.…

Astrophysics · Physics 2009-11-06 Rita M. Sambruna , C. Megan Urry , F. Tavecchio , L. Maraschi , R. Scarpa , G. Chartas , T. Muxlow

We present new Chandra observations of 21 z>4 quasars, including 11 sources at z>5. These observations double the number of X-ray detected quasars at z>5, allowing investigation of the X-ray spectral properties of a substantial sample of…

This letter reports rich X-ray jet structures found in the Chandra observation of PKS 1055+201. In addition to an X-ray jet coincident with the radio jet we detect a region of extended X-ray emission surrounding the jet as far from the core…

Two relativistic X-ray jets have been detected with the Chandra X-ray observatory from the black hole X-ray transient XTE J1550-564. We report a full analysis of the evolution of the two jets with a gamma-ray burst external shock model. A…

Astrophysics · Physics 2012-09-13 Shuang-Nan Zhang , JingFang Hao

We report the discovery of five gravitationally lensed quasars from the Sloan Digital Sky Survey (SDSS). All five systems are selected as two-image lensed quasar candidates from a sample of high-redshift (z>2.2) SDSS quasars. We confirmed…

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

For the interpretation of X-ray radiation from kiloparsec jets of quasars, the inverse Compton scattering of the cosmic microwave background has been widely used for almost 20 years. A recent analysis of the Fermi-LAT observational data…

High Energy Astrophysical Phenomena · Physics 2020-12-10 M. S. Butuzova , A. B. Pushkarev , E. S. Shablovinskaya , S. V. Nazarov

We present the X-ray analysis of a deep ~200 ksec Chandra observation of the compact steep spectrum radio-loud quasar 3C 186 (z=1.06) and investigate the contribution of the unresolved radio jet to the total X-ray emission. The spectral…

High Energy Astrophysical Phenomena · Physics 2015-06-04 G. Migliori , A. Siemiginowska , A. Celotti

We propose that the X-ray emission detected by Chandra from the 100-kiloparsec-scale jet of PKS 0637-752 is produced through inverse Compton scattering of the Cosmic Microwave Background (CMB). We analyze the physical state of the jet and…

Astrophysics · Physics 2009-10-31 F. Tavecchio , L. Maraschi R. M. Sambruna , C. M. Urry