0000000000329715

AUTHOR

P. R. Burd

showing 2 related works from this author

LOFAR measures the hotspot advance speed of the high-redshift blazar S5 0836+710

2019

Our goal is to study the termination of an AGN jet in the young universe and to deduce physical parameters of the jet and the intergalactic medium. We use LOFAR to image the long-wavelength radio emission of the high-redshift blazar S5 0836+710 on arcsecond scales between 120 MHz and 160 MHz. The LOFAR image shows a compact unresolved core and a resolved emission region about 1.5 arcsec to the southwest of the radio core. This structure is in general agreement with previous higher-frequency radio observations with MERLIN and the VLA. The southern component shows a moderately steep spectrum with a spectral index of about $\gtrsim -1$ while the spectral index of the core is flat to slightly i…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSpectral indexActive galactic nucleusProper motion010308 nuclear & particles physicsRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLOFARAstrophysics - Astrophysics of Galaxies01 natural sciencesRedshiftSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencesIntergalactic travelAstrophysics - High Energy Astrophysical PhenomenaBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsAstronomy & Astrophysics
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TANAMI: Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry - II. Additional Sources

2018

TANAMI is a multiwavelength program monitoring active galactic nuclei (AGN) south of -30deg declination including high-resolution Very Long Baseline Interferometry (VLBI) imaging, radio, optical/UV, X-ray and gamma-ray studies. We have previously published first-epoch 8.4GHz VLBI images of the parsec-scale structure of the initial sample. In this paper, we present images of 39 additional sources. The full sample comprises most of the radio- and gamma-ray brightest AGN in the southern quarter of the sky, overlapping with the region from which high-energy (>100TeV) neutrino events have been found. We characterize the parsec-scale radio properties of the jets and compare with the quasi-simu…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Active galactic nucleus010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio telescopeNeutrino detector13. Climate actionSpace and Planetary Science0103 physical sciencesVery-long-baseline interferometryNeutrinoBlazarAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsFermi Gamma-ray Space Telescope
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