MYSTIC: a high angular resolution K-band imager at CHARA

This is the final version. Available on open access from SPIE via the DOI in this recordData, Materials, and Code Availability: The data reduction pipeline is available at https://gitlab.chara.gsu.edu/lebouquj/mircx_pipeline/Much of this manuscript originally appeared in SPIE Proceedings Volume 12183, Optical and Infrared Interferometry and Imaging VIII; 121830B (2022) https://doi.org/10.1117/12.2629437; available in ORE at http://hdl.handle.net/10871/131161The Michigan Young Star Imager at CHARA (MYSTIC) is a K-band interferometric beam combining instrument funded by the U.S. National Science Foundation, designed primarily for imaging sub-au scale disk structures around nearby young stars and to probe the planet formation process. Installed at the CHARA Array in July 2021, with baselines up to 331 m, MYSTIC provides a maximum angular resolution of λ / 2B ∼ 0.7 mas. The instrument injects phase-corrected light from the array into inexpensive, single-mode, polarization maintaining silica fibers, which are then passed via a vacuum feedthrough into a cryogenic dewar operating at 220 K for imaging. MYSTIC uses a high frame rate, ultra-low read noise SAPHIRA detector and implements two beam combiners: a six-telescope image plane beam combiner, based on the MIRC-X design, for targets as faint as 7.7 Kmag, as well as a four-telescope integrated optic beam-combiner mode using a spare chip leftover from the GRAVITY instrument. MYSTIC is co-phased with the MIRC-X (J + H band) instrument for simultaneous fringe-tracking and imaging and shares its software suite with the latter to allow a single observer to operate both instruments. We present the instrument design, review its operational performance, present early commissioning science observations, and propose upgrades to the instrument that could improve its K-band sensitivity to 10th magnitude in the near future.USA National Science Foundation Advanced Technologies and Instrumentation ProgramEuropean Union Horizon 2020NASA-XRPNSF-ASTNASA-MSGCNASAEuropean Research Council (ERC)Science and Technology Facilities Council (STFC