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20002026
most citedLarge scale jets in AGN: multiwavelength mapping

293 citations · 2.2k across the 66 of their papers we have counts for

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8 papers · 1 filter

astro-ph.HE2024★ 11 cited

The case for super-Eddington accretion in JWST broad-line AGN during the first billion years

Erini Lambrides, Rebecca Larson, Kristen Garofali +23

A multitude of JWST studies reveal a surprising over-abundance of over-massive accreting super-massive black holes (SMBHs) -- leading to a deepening tension between theory and obse…

astro-ph.HE2023★ 1 cited

Constraints on the narrow-line region of the X-ray quasi-periodic eruption source GSN 069

Kishore C. Patra, Wenbin Lu, Yilun Ma +4

The origins of quasi-periodic eruptions (QPEs) are poorly understood, although most theoretical explanations invoke an accretion disk around a supermassive black hole. The gas and…

astro-ph.HE2023★ 9 cited

Variability of extragalactic X-ray jets on kiloparsec scales

Eileen T. Meyer, Aamil Shaik, Yanbo Tang +10

Unexpectedly strong X-ray emission from extragalactic radio jets on kiloparsec scales has been one of the major discoveries of Chandra, the only X-ray observatory capable of sub-ar…

astro-ph.HE2020★ 17 cited

TXS 2116077: A Gamma-ray Emitting Relativistic Jet Hosted in a Galaxy Merger

Vaidehi S. Paliya, Enrique Pérez, Rubén García-Benito +10

What triggers collimated relativistic outflows or jets, from the centers of galaxies remains a fundamental question in astrophysics. The merging of two galaxies has been proposed t…

astro-ph.HE2012★ 54 cited

Chandra Observations of 3C Radio Sources with z<0.3 II: completing the snapshot survey

F. Massaro, G. R. Tremblay, D. E. Harris +14

We report on the second round of Chandra observations of the 3C snapshot survey developed to observe the complete sample of 3C radio sources with z<0.3 for 8 ksec each. In the firs…

astro-ph.HE2010★ 66 cited

Chandra Observations of 3C Radio Sources with z<0.3: Nuclei, Diffuse Emission, Jets and Hotspots

F. Massaro, D. E. Harris, G. Tremblay +11

We report on our Chandra Cycle 9 program to observe half of the 60 (unobserved by Chandra) 3C radio sources at z<0.3 for 8 ksec each. Here we give the basic data: the X-ray intensi…