Exo-NINJA at Subaru: fiber-fed spectro-imaging of exoplanets and circumstellar disks at R$\sim$4000
Mona El Morsy, Julien Lozi, Olivier Guyon, Thayne Currie, S\'ebastien, Vievard, Julia Bryant, Chihiro Tokoku, Vincent Deo, Kyohoon Ahn, Fred Crous,, Adeline Haobing Wang, Zinat Mahol Sathi

TL;DR
Exo-NINJA is a planned fiber-fed spectro-imaging instrument for the Subaru Telescope that will enable high-resolution, spatially-resolved characterization of exoplanets and circumstellar disks in the near-infrared, with significantly improved throughput.
Contribution
It introduces a novel fiber-fed spectro-imaging system linking high contrast imaging and medium-resolution spectroscopy at Subaru, enhancing throughput and spatial resolution for exoplanet studies.
Findings
Design and integration plan for Exo-NINJA at Subaru.
Laboratory tests of fiber bundle throughput and focal ratio degradation.
Expected on-sky performance and trade-offs for fiber choices.
Abstract
Exo-NINJA will realize nearIR R4000 diffraction-limited narrow-field spectro-imaging for characterization of exoplanets and circumstellar disk structures. It uniquely combines mid-R spectroscopy, high throughput, and spatial resolution, in contrast to CHARIS, which does spectro-imaging, and REACH, which is single-point (no spatial resolution). Exo-NINJA's spectro-imaging at the telescope diffraction limit will characterize exoplanet atmospheres, detect and map (spatially and spectrally) gas accretion on protoplanets, and also detect exoplanets at small angular separation (/D) from their host star by spectro-astrometry. Exo-NINJA will link two instruments at the Subaru Telescope using a high-throughput hexagonal multi-mode fiber bundle (hexabundle). The fiber coupling resides between the high contrast imaging system SCExAO, which combines ExAO and coronagraph, and the…
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