VASCO provides the first fully automated CASA pipeline for blind calibration of heterogeneous archival VLBA VLBI data, succeeding on 97.8% of 1000 test sources across multiple bands from 1995-2023.
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5 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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A propagating jet disturbance in 3C 120 produces an orphan gamma-ray flare by inverse-Compton scattering synchrotron photons from a stationary feature at about 10 times the broad-line region radius.
VLBI imaging at 4.9-43.2 GHz resolves symmetric parabolically expanding twin jets in 3C 452 to a few thousand Schwarzschild radii, with low Doppler factors indicating a viewing angle of about 70 degrees.
High-resolution radio imaging shows TGSSJ1530+1049 as a ~5.5 kpc medium-sized symmetric object whose lobes align with but do not reach the full extent of the ionized gas seen by JWST in a dense z=4 environment.
Spectral index maps of the limb-brightened jet in 3C 84 show significant evolution across three epochs, indicating dynamic filamentary structures, evolving magnetic fields, and interaction with the ambient medium.
citing papers explorer
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VASCO: A fully automated CASA pipeline for large volume VLBI data calibration
VASCO provides the first fully automated CASA pipeline for blind calibration of heterogeneous archival VLBA VLBI data, succeeding on 97.8% of 1000 test sources across multiple bands from 1995-2023.
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A Ring of Fire Orphan {\gamma}-Ray Flare in the Neutrino Candidate 3C 120
A propagating jet disturbance in 3C 120 produces an orphan gamma-ray flare by inverse-Compton scattering synchrotron photons from a stationary feature at about 10 times the broad-line region radius.
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The twin-jet system in the FRII radio galaxy 3C 452: A sub-parsec scale VLBI study
VLBI imaging at 4.9-43.2 GHz resolves symmetric parabolically expanding twin jets in 3C 452 to a few thousand Schwarzschild radii, with low Doppler factors indicating a viewing angle of about 70 degrees.
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High-resolution radio imaging of TGSSJ1530+1049, a radio galaxy in a dense environment at z=4
High-resolution radio imaging shows TGSSJ1530+1049 as a ~5.5 kpc medium-sized symmetric object whose lobes align with but do not reach the full extent of the ionized gas seen by JWST in a dense z=4 environment.
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Spectral index evolution of the limb-brightened jet in 3C 84
Spectral index maps of the limb-brightened jet in 3C 84 show significant evolution across three epochs, indicating dynamic filamentary structures, evolving magnetic fields, and interaction with the ambient medium.