| Issue |
A&A
Volume 711, July 2026
|
|
|---|---|---|
| Article Number | A201 | |
| Number of page(s) | 17 | |
| Section | Astronomical instrumentation | |
| DOI | https://doi.org/10.1051/0004-6361/202557010 | |
| Published online | 14 July 2026 | |
Multi-map holography for large crossed-Dragone telescopes
1
I. Physikalisches Institut, Universität zu Köln,
Zülpicher Straße 77,
50937
Köln,
Germany
2
Cavendish Laboratory, University of Cambridge,
Cambridge
CB3 0HE,
UK
3
Max Planck Institute for Radio Astronomy,
Bonn,
Germany
4
Departamento de Astronomía, Universidad de Chile,
Santiago
7591245,
Chile
5
Departamento de Ingeniería Eléctrica, Universidad de Chile,
Santiago
8370451,
Chile
6
School of Engineering and Natural Sciences, University of Iceland,
107
Reykjavík,
Iceland
7
Instituto de Astrofísica and Centro de Astro-Ingeniería, Facultad de Física, Pontificia Universidad Católica de Chile,
Santiago,
Chile
8
National Radio Astronomy Observatory, Central Development Laboratory,
Charlottesville,
VA
22903
USA
★ Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
27
August
2025
Accepted:
8
June
2026
Abstract
We present a novel microwave holography technique for large crossed-Dragone telescopes, which feature two similarly sized off-axis reflectors whose surface deformations must be measured and corrected independently. A major challenge in these systems is the degeneracy of wavefront distortions caused by surface errors on both reflectors, which conventional single-beam holography cannot effectively disentangle. The method addresses this challenge by acquiring five beam maps at distinct focal plane positions and employing an inference-based analysis to reconstruct the individual surface error distributions of the two large reflectors. We developed a fast and accurate beam analysis method based on the Fresnel-Kirchhoff diffraction theorem to accelerate the forward beam calculations. This greatly reduces the computational cost while maintaining high accuracy, enabling a practical application to iterative fittings for the large crossed-Dragone telescopes. The accuracy and feasibility of the new technique have been verified by numerical simulations for the FYST telescope and experimental tests for a 400 mm diameter crossed-Dragone optics.
Key words: methods: analytical / methods: numerical / site testing / space vehicles: instruments / telescopes
Deceased: June 2022. This work is dedicated to his memory.
© The Authors 2026
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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