Bringing high-spectral resolution to VLT/SPHERE with a fibre coupling to VLT/CRIRES+
A. Vigan, G. P. P. L. Otten, E. Muslimov, K. Dohlen, M. W. Phillips,, U. Seemann, J.-L. Beuzit, R. Dorn, M. Kasper, D. Mouillet, I. Baraffe, A., Reiners

TL;DR
This paper proposes a novel system combining VLT/SPHERE and VLT/CRIRES+ to enable high-spectral resolution studies of exoplanets, overcoming current limitations in spectral resolution and spatial resolution for direct imaging.
Contribution
It introduces the HiRISE project, a demonstrator integrating high-contrast imaging with high-resolution spectroscopy using fiber coupling, advancing exoplanet characterization capabilities.
Findings
Simulations demonstrate potential for improved exoplanet spectral analysis.
Preliminary fiber injection design shows feasibility for integration.
Expected enhancement in understanding exoplanet formation and composition.
Abstract
Atmospheric composition provides essential markers of the most fundamental properties of giant exoplanets, such as their formation mechanism or internal structure. New-generation exoplanet imagers, like VLT/SPHERE or Gemini/GPI, have been designed to achieve very high contrast (>15 mag) at small angular separations (0.5\as) for the detection of young giant planets in the near-infrared, but they only provide very low spectral resolutions () for their characterization. High-dispersion spectroscopy at resolutions up to is one of the most promising pathways for the detailed characterization of exoplanets, but it is currently out of reach for most directly imaged exoplanets because current high-dispersion spectrographs in the near-infrared lack coronagraphs to attenuate the stellar signal and the spatial resolution necessary to resolve the planet. Project HiRISE…
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Taxonomy
TopicsSpectroscopy and Laser Applications · Adaptive optics and wavefront sensing · Atmospheric and Environmental Gas Dynamics
