Mobile Intensity Interferometer for Stellar Observations (MI$^2$SO)
Christopher Ingenh\"utt (1), Pedro Batista (1), Gisela Anton (1), Alison Mitchell (1), Naomi Vogel (1), Adrian Zink (1), Andreas Zmija (1,2), Stefan Funk (1) ((1) Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universit\"at Erlangen-N\"urnberg, Erlangen, Germany

TL;DR
This paper presents a novel, portable intensity interferometer using Fresnel lenses for stellar observations, successfully measuring the angular diameter of Arcturus with high precision in a short observation time.
Contribution
It introduces a lightweight, scalable, and mobile intensity interferometer design tailored for stellar measurements, demonstrating its effectiveness through a successful observation campaign.
Findings
Measured Arcturus's angular diameter with milliarcsecond accuracy
Demonstrated the interferometer's capability with less than 11 hours of observation
Validated the design's potential for targeted stellar observations
Abstract
In recent years, intensity interferometry has seen renewed interest and successful application at Imaging Atmospheric Cherenkov Telescope arrays. These measurements are usually performed during bright moon periods while the instruments' primary purpose -- gamma-ray observations -- cannot be fulfilled. The Mobile Intensity Interferometer for Stellar Observations was designed as a proof of concept for a purpose-built intensity interferometer. Using acrylic Fresnel lenses 1 m in diameter with 1.2 m focal length, a compact, economical and lightweight design was realised. The detector fixture allows for translation in the z-axis to adjust for measurements at different wavelengths (and therefore focal points) and easy swapping of the detector in its entirety. Both mobility and scalability in quantity of this design allow for specific targeting of projected baselines and orientations based on…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Superconducting and THz Device Technology · Adaptive optics and wavefront sensing
