Prospects of using closure traces directly for imaging in Very Long Baseline Interferometry
Hendrik M\"uller

TL;DR
This paper investigates the potential of using closure traces directly for imaging in Very Long Baseline Interferometry, highlighting their advantages and limitations, especially for future larger arrays like the next-generation EHT.
Contribution
It introduces a novel imaging pipeline using closure traces, analyzes their degeneracies, and assesses their feasibility for current and future VLBI configurations.
Findings
Closure traces are independent of gains and leakages.
Direct imaging from closure traces is limited for 2017 EHT but feasible for larger arrays.
Multiobjective techniques are necessary to handle multimodal solutions.
Abstract
The reconstruction of the polarization of a source in radio interferometry is a challenging calibration problem since the reconstruction strongly depends on the gains and leakages that need to be inferred along with the image. This is particularly true for the Event Horizon Telescope (EHT) due to its small number of antennas, small signal-to-noise ratio and large gain corruptions. To recover linear polarization, one either has to infer the leakages and gains together with the image structure, or rely completely on calibration independent closure quantities. While the first approach has been explored in Very Long Baseline Interferometry (VLBI) for a long time, the later one has been less studied for polarimetry. Closure traces are a recently proposed concept of closure quantities that, in contrast to closure phases and closure amplitudes, are independent against both gains and leakages…
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