| Issue |
A&A
Volume 703, November 2025
|
|
|---|---|---|
| Article Number | A196 | |
| Number of page(s) | 14 | |
| Section | Numerical methods and codes | |
| DOI | https://doi.org/10.1051/0004-6361/202556838 | |
| Published online | 18 November 2025 | |
VIPCALs: A fully automated calibration pipeline for very long baseline interferometry data
1
Institute of Astrophysics, Foundation for Research and Technology – Hellas,
N. Plastira 100,
Voutes
70013
Heraklion,
Greece
2
Department of Physics, University of Crete,
70013
Heraklion,
Greece
3
Department of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University,
PO Box 9010,
6500 GL
Nijmegen,
The Netherlands
★ Corresponding author: dalvarez@physics.uoc.gr
Received:
12
August
2025
Accepted:
7
October
2025
Context. Very long baseline interferometry (VLBI) is a powerful observational technique that can achieve sub-milliarcsecond resolution. However, it requires complex and often manual post-correlation calibration to correct for instrumental, geometric, and propagation-related errors. Unlike connected-element interferometers, VLBI arrays typically deliver raw visibilities rather than science-ready data, and existing pipelines are largely semi-automated and reliant on user supervision.
Aims. We aim to develop and validate a fully automated, end-to-end calibration pipeline for continuum VLBI data that operates without human intervention or prior knowledge of the dataset. The pipeline must be scalable to thousands of sources and suitable for heterogeneous archival observations, as required by initiatives such as the Search for Milli-Lenses (SMILE) project.
Methods. We present the VLBI Pipeline for automated data Calibration using AIPS, or VIPCALs. Implemented in Python using ParselTongue, VIPCALs reproduces the standard AIPS calibration workflow in a fully unsupervised mode. The pipeline carries out data import, retrieval of system temperature and gain curve data, ionospheric and geometric corrections, fringe fitting, and amplitude and bandpass calibration steps. VIPCALs performs automatic reference antenna selection and calibrator identification, and it generates diagnostic outputs for inspection. It can be easily used through a simple graphical user interface. We validated VIPCALs on a representative sample of Very Long Baseline Array (VLBA) data corresponding to 1000 sources from the SMILE project.
Results. VIPCALs successfully calibrated observations of 955 of the 1000 test sources across multiple frequency bands. Over 91% of the calibrated datasets achieved successful fringe fitting on target in at least half of the solutions attempted. The median ratio of calibrated visibilities to initial total visibilities was 0.87. The average processing time was below 10 minutes per dataset when using a single-core configuration, demonstrating both efficiency and scalability.
Conclusions. VIPCALs enables robust, reproducible, and fully automated calibration of VLBI continuum data, significantly lowering the entry barrier for VLBI science and making large-scale projects such as SMILE feasible.
Key words: atmospheric effects / instrumentation: interferometers / methods: data analysis / radio continuum: general
Publisher note: The email address of the corresponding author was corrected on 21 November 2025.
© The Authors 2025
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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