infrastructure
ALMA's Hardest Polarization Data Got a Public Loading Dock
VAPOLA turns specialized phased-array observations of active galaxies and the Galactic center into science-ready products.
Summary
VAPOLA turns specialized phased-array observations of active galaxies and the Galactic center into science-ready products.
The VAPOLA repository uses an automated pipeline to create calibrated visibilities, full-Stokes images, polarization and spectral-index maps, fitted parameters and calibration metadata from ALMA observations made during global very-long-baseline campaigns. The first release lowers the expertise barrier for work on jets, accretion flows and Sgr A*. Its value is reusable infrastructure; scientific conclusions still depend on each analysis.
Why it matters
VAPOLA turns specialized phased-array observations of active galaxies and the Galactic center into science-ready products.
Limits and context
No additional limitation was separately recorded.
Key claims
VAPOLA turns specialized phased-array observations of active galaxies and the Galactic center into science-ready products.
Evidence: source-2026-08-03-013
Sources
- Astronomy & Astrophysics: VAPOLA ALMA polarization archiveEDP Sciences · secondary reporting
Corrections
No corrections have been recorded for this story.