Presentation + Paper
28 August 2024 The Big Fringe Telescope
Author Affiliations +
Abstract
The Big Fringe Telescope (BFT) is a facility concept under development for a next-generation, kilometer-scale optical interferometer. Observations over the past two decades from routinely operational facilities such as CHARA and VLTI have produced groundbreaking scientific results, reflecting the mature state of the techniques in optical interferometry. However, routine imaging of bright main sequence stars remains a surprisingly unexplored scientific realm. Additionally, the three-plus decade old technology infrastructure of these facilities leads to high operations & maintenance costs, and limits performance. We are developing the BFT, based upon robust, modern, commercially-available, automated technologies with low capital construction and O&M costs, in support of kilometer-scale optical interferometers that will open the door to regular ‘snapshot’ imaging of main sequence stars. Focusing on extreme angular resolution for bright objects leads to substantial reductions in expected costs through use of COTS elements and simplified infrastructure.
Conference Presentation
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gerard T. van Belle and Anders M. Jorgensen "The Big Fringe Telescope", Proc. SPIE 13095, Optical and Infrared Interferometry and Imaging IX, 130951R (28 August 2024); https://doi.org/10.1117/12.3020515
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KEYWORDS
Telescopes

Stars

Astronomical imaging

Optical interferometry

Exoplanets

Astronomical interferometers

Astronomical interferometry

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