activity
19962019
most citedA Chandra Survey of Quasar Jets: First Results

151 citations · 1.5k across the 45 of their papers we have counts for

collaborators

46 papers

astro-ph.IM2019★ 17 cited

Venus Express radio occultation observed by PRIDE

T. M. Bocanegra-Bahamon, G. Molera Calves, L. I. Gurvits +18

Context. Radio occultation is a technique used to study planetary atmospheres by means of the refraction and absorption of a spacecraft carrier signal through the atmosphere of the…

astro-ph.HE2018★ 36 cited

An X-ray Imaging Survey of Quasar Jets -- The Complete Survey

H. L. Marshall, J. M. Gelbord, D. M. Worrall +8

We present Chandra X-ray imaging of a flux-limited sample of flat spectrum radio-emitting quasars with jet-like structure. X-rays are detected from 59% of 56 jets. No counterjets w…

astro-ph.IM2017★ 27 cited

VLBI ecliptic plane survey: VEPS-1

Fengchun Shu, Leonid Petrov, Wu Jiang +12

We present here the results of the first part of the VLBI Ecliptic Plane Survey (VEPS) program. The goal of the program is to find all compact sources within of the ecl…

astro-ph.HE2016★ 25 cited

The TANAMI Multiwavelength Program: Dynamic SEDs of Southern Blazars

Felicia Krauß, Joern Wilms, Matthias Kadler +32

Simultaneous broadband spectral and temporal studies of blazars are an important tool for investigating active galactic nuclei (AGN) jet physics. We study the spectral evolution be…

astro-ph.IM2016★ 3 cited

Progress on VLBI Ecliptic Plane Survey

Fengchun Shu, Leonid Petrov, Wu Jiang +5

We launched the VLBI Ecliptic Plane Survey program in 2015. The goal of this program is to find all compact sources within 7.5 degrees of the ecliptic plane which are suitable as p…

astro-ph.HE2015★ 71 cited

Ruling out IC/CMB X-rays in PKS 0637-752 and the Implications for TeV Emission from Large-Scale Quasar Jets

Eileen T. Meyer, Markos Georganopoulos, William B. Sparks +3

The Chandra X-ray observatory has discovered dozens of resolved, kiloparsec-scale jets associated with powerful quasars in which the X-ray fluxes are observed to be much higher tha…