Poster
13 December 2020 High-spectral resolution interferometry at 1 micrometer with VLTI/BIFROST: science drivers and instrument design
Author Affiliations +
Conference Poster
Abstract
We present science cases and instrument design considerations for a short-wavelength (Y/J-band), high spectral dispersion (R=25,000) instrument that could be implemented at the VLTI visitor focus. The instrument will unlock powerful venues for studying accretion and mass-loss processes at the early/late stages of stellar evolution, for detecting accreting protoplanets around young stars, and for probing the spin-orbit alignment in directly-imaged planetary systems and multiple star systems. In conjuncture with infrastructure improvements on the VLTI unit telescopes, the instrument will also enable off-axis spectroscopy of exoplanets in the 0.1-2” separation range, enabling high-SNR, high spectral resolution follow-up of exoplanets detected with ELT/JWST. We discuss technical implementations, including on fringe tracking and fast laboratory low-order adaptive optics. We outline a pathway for implementation and stress possible synergies with other instruments in the proposed ASGARD suite.
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stefan Kraus, Michael J. Ireland, Jean-Baptiste Le Bouquin, John D. Monnier, Barnaby Norris, Frantz Martinache, Denis Defrère, and Narsireddy Anugu "High-spectral resolution interferometry at 1 micrometer with VLTI/BIFROST: science drivers and instrument design", Proc. SPIE 11446, Optical and Infrared Interferometry and Imaging VII, 114462H (13 December 2020); https://doi.org/10.1117/12.2562181
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KEYWORDS
Spectral resolution

Interferometry

Stars

Exoplanets

Adaptive optics

Diagnostics

James Webb Space Telescope

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