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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3 Pith papers cite this work, alongside 110 external citations. Polarity classification is still indexing.
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CRF-K-2025 is a new K-band VLBI catalog of 1317 sources with median position uncertainties of 60 μas in RA and 104 μas in Dec, 25% better than ICRF3-K and comparable to ICRF3-SX.
SKA-Low can characterise mid-latitude ionospheric structure via multiple interferometric phase-screen and scintillation methods, with forward modelling linking observables to physical plasma conditions.
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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The Celestial Reference Frame at K Band: The CRF-K-2025 Catalog
CRF-K-2025 is a new K-band VLBI catalog of 1317 sources with median position uncertainties of 60 μas in RA and 104 μas in Dec, 25% better than ICRF3-K and comparable to ICRF3-SX.
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Methods of Observing and Characterising the Ionosphere with SKA-Low
SKA-Low can characterise mid-latitude ionospheric structure via multiple interferometric phase-screen and scintillation methods, with forward modelling linking observables to physical plasma conditions.