Poster
13 December 2020 Visible interferometry at the VLTI
Florentin Millour, Fabien Patru, Andrea Chiavassa, Anthony Meilland, Marc-Antoine Martinod, Denis Mourard, Philippe Stee
Author Affiliations +
Conference Poster
Abstract
Time has come for the VLTI to prepare its jump into the visible domain, revealing many physical processes occuring in stars, planets and galaxies. Visible interferometry has a superior angular resolution than its IR siblings with the same baselines. Science with a visible VLTI ranges from evolved stars mass loss, fundamental parameters of main sequence stars, surface-brightness relation refinement, and the progenitors of gravitational waves ... These critical science cases are becoming feasible thanks to recent instrumental improvements: better detectors, adaptive optics, fringe trackers, use of optical fibers and integrated optics. The appeal for visible light at VLTI is now stronger than ever because IR has already been explored substantially at ESO. This presentation further addresses possible path forward toward a visible instrument with scientific-driven specifications. We will discuss the benefits of a survey-type observing program to allow it to operate at its full potential.
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Florentin Millour, Fabien Patru, Andrea Chiavassa, Anthony Meilland, Marc-Antoine Martinod, Denis Mourard, and Philippe Stee "Visible interferometry at the VLTI", Proc. SPIE 11446, Optical and Infrared Interferometry and Imaging VII, 114462C (13 December 2020); https://doi.org/10.1117/12.2562269
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KEYWORDS
Interferometry

Stars

Visible radiation

Adaptive optics

Galactic astronomy

Optical fibers

Optical tracking

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