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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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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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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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.