VLBI data on TXS 2005+403 show refractive substructure from interstellar turbulence that cannot be explained by diffractive scattering alone and remains stable over nine years.
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6 Pith papers cite this work, alongside 45 external citations. Polarity classification is still indexing.
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VLBI monitoring reveals a 21c apparent speed in TXS 0506+056, interpreted as evidence for a stratified jet with Gamma>20 spine that accounts for neutrino production and radio flare timing.
CSO-2 radio lobes sit near minimum-energy magnetic fields of ~20 mG, implying rapid GHz fading post-jet-shutoff and massive-star origins for luminous sources.
SKA VLBI surveys of the Southern sky will support geodesy with a Southern network, increase compact source density for calibration, extend the celestial reference frame, and enable high-precision astrometry for astrophysics.
High-precision VLBI detects 250 μas core shift between 8.4 and 43.2 GHz in BL Lacertae, with fitted index k_r = 1.18 consistent with equipartition.
AGN (jetted and non-jetted) are viable high-energy neutrino sources, with TXS 0506+056 and NGC 1068 as the only statistically significant associations so far, while gamma-ray blazars contribute only a small fraction of the diffuse flux.
citing papers explorer
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Direct VLBI Detection of Interstellar Turbulence Imprint on a Quasar: TXS 2005+403
VLBI data on TXS 2005+403 show refractive substructure from interstellar turbulence that cannot be explained by diffractive scattering alone and remains stable over nine years.
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A hidden ultra-relativistic spine in the jet of a neutrino-associated blazar
VLBI monitoring reveals a 21c apparent speed in TXS 0506+056, interpreted as evidence for a stratified jet with Gamma>20 spine that accounts for neutrino production and radio flare timing.
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Minimum Energies and Magnetic Field Strengths of Edge-brightened Compact Symmetric Objects
CSO-2 radio lobes sit near minimum-energy magnetic fields of ~20 mG, implying rapid GHz fading post-jet-shutoff and massive-star origins for luminous sources.
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SKA VLBI survey of the Southern sky for astrometry, geodesy, and astrophysics
SKA VLBI surveys of the Southern sky will support geodesy with a Southern network, increase compact source density for calibration, extend the celestial reference frame, and enable high-precision astrometry for astrophysics.
-
Detections of nearly bias-free core shifts with 5-30 $\mu$as precisions at 8-43 GHz in BL Lacertae
High-precision VLBI detects 250 μas core shift between 8.4 and 43.2 GHz in BL Lacertae, with fitted index k_r = 1.18 consistent with equipartition.
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Active Galactic Nuclei as high-energy neutrino sources
AGN (jetted and non-jetted) are viable high-energy neutrino sources, with TXS 0506+056 and NGC 1068 as the only statistically significant associations so far, while gamma-ray blazars contribute only a small fraction of the diffuse flux.