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On Optimal Geometry for Space Interferometers

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arxiv 2305.19072 v2 pith:X3AZXOSP submitted 2023-05-30 astro-ph.IM

A. G. Rudnitskiy , M. A. Shchurov , S. V. Chernov , T. A. Syachina , P. R. Zapevalin This is my paper · ORCID
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abstract

This paper examines options for orbit configurations for a space interferometer. In contrast to previously presented concepts for space very long baseline interferometry, we propose a combination of regular and retrograde near-Earth circular orbits in order to achieve a faster filling of $(u,v)$ coverage. With the rapid relative motion of the telescopes, it will be possible to quickly obtain high quality images of supermassive black holes. As a result of such an approach, it will be possible for the first time to conduct high quality studies of the supermassive black hole close surroundings in dynamics.

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  1. Method for Determining the Parameters of a Ring-like Structure from the Visibility Function Shape

    astro-ph.IM 2025-02 conditional novelty 4.0 of 10

    A method to measure ring diameter, width, and asymmetry from the zeros of the interferometric visibility function is derived and tested on M87*, yielding r≈23 μas and B=0.48.

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