Photonic beam-combiner for visible interferometry with SCExAO/FIRST: laboratory characterization and design optimization
Manon Lallement, Elsa Huby, Sylvestre Lacour, Guillermo Martin, Kevin, Barjot, Guy Perrin, Daniel Rouan, Vincent Lapeyrere, Sebastien Vievard,, Olivier Guyon, Julien Lozi, Vincent Deo, Takayuki Kotani, Cecil Pham, Cedric, Cassagnettes, Adrien Billat, Nick Cvetojevic

TL;DR
This paper reports on the development and laboratory testing of a photonic integrated circuit for visible interferometry, aiming to improve stability and sensitivity in astronomical measurements, specifically for the FIRST project.
Contribution
It introduces optimized designs of a visible PIC for interferometry, including experimental characterization and theoretical modeling of different combiner architectures.
Findings
Successful laboratory characterization of waveguides.
Optimized designs for symmetric and asymmetric combiners.
Potential for improved stability and sensitivity in astronomical interferometry.
Abstract
Integrated optics are used to achieve astronomical interferometry inside robust and compact materials, improving the instrument's stability and sensitivity. In order to perform differential phase measurements at the H line (656.3 nm) with the 600-800 nm spectro-interferometer FIRST, a photonic integrated circuit (PIC) is being developed in collaboration with TEEM Photonics. This PIC performs the interferometric combination of the beams coming from sub-apertures selected in the telescope pupil, thus implementing the pupil remapping technique to restore the diffraction limit of the telescope. In this work, we report on the latest developments carried out within the FIRST project to produce a high performance visible PIC. The PICs are manufactured by TEEM Photonics, using their technology based on ion exchange in glass. The first part of the study consists in the…
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