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researcher

T. G. Arshakian

5 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author4
  • middle author1

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO3
  • astro-ph1
  • astro-ph.GA1
ORCID 0000-0003-0318-3247

identity via Semantic Scholar / OpenAlex

activity
20042011
most citedRelativistic plasma as the dominant source of the optical continuum emission in the broad-line radio galaxy 3C 120

50 citations · 118 across the 5 of their papers we have counts for

collaborators
Showing 2011Show all

2 papers · 1 filter

astro-ph.CO2011★ 32 cited

Radio-Optical-Gamma-Ray properties of MOJAVE AGN detected by Fermi/LAT

T. G. Arshakian, J. León-Tavares, M. Boettcher +5

Aims. We use a sample of 83 core-dominated active galactic nuclei (AGN) selected from the MOJAVE (Monitoring of Jets in AGN with VLBA Experiments) radio-flux-limited sample and det…

astro-ph.CO2011★ 11 cited

Modeling the total and polarized emission in evolving galaxies: "spotty" magnetic structures

T. G. Arshakian, R. Stepanov, R. Beck +2

Future radio observations with the SKA and its precursors will be sensitive to trace spiral galaxies and their magnetic field configurations up to redshift z≈3. We suggest…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.