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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
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.
citing papers explorer
-
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.
-
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.