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
4 Pith papers cite this work. Polarity classification is still indexing.
representative citing papers
EHT data show a 51.8 microarcsecond ring around Sgr A* consistent with the shadow of a 4 million solar mass Kerr black hole viewed at moderate inclination.
A tiered observational strategy is outlined to identify planetary-scale broadband radio technosignatures (BRaTs) from advanced civilizations up to 100 pc away using multi-parameter diagnostics to separate them from natural signals.
Observational case study of PSR J2338+4818 providing updated timing, single-pulse statistics from 27,228 detections, and scintillation parameters with no detected nulling.
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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First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
EHT data show a 51.8 microarcsecond ring around Sgr A* consistent with the shadow of a 4 million solar mass Kerr black hole viewed at moderate inclination.
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Isolating Broadband Radio Technosignatures (BRaTs): A Framework for Detecting Planetary-Scale Leakage
A tiered observational strategy is outlined to identify planetary-scale broadband radio technosignatures (BRaTs) from advanced civilizations up to 100 pc away using multi-parameter diagnostics to separate them from natural signals.
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A Pilot Study of Mildly Recycled Pulsars: A Case Study of PSR J2338+4818
Observational case study of PSR J2338+4818 providing updated timing, single-pulse statistics from 27,228 detections, and scintillation parameters with no detected nulling.