WST -- Widefield Spectroscopic Telescope: addressing the instrumentation challenges of a new 12m class telescope dedicated to widefield Multi-object and Integral Field Spectroscopy
David Lee, Joel D. R. Vernet, Roland Bacon, Alexandre Jeanneau,, Ernesto Oliva, Anna Brucalassi, Andrea Tozzi, Jos\'e A. Araiza-Dur\'an,, Andrea Bianco, Jan Kragt, Ramon Navarro, Bianca Garilli, Kjetil Dohlen,, Jean-Paul Kneib, Ricardo Araujo, Maxime Rombach, Eloy Hernandez

TL;DR
The paper discusses the design and instrumentation challenges of a proposed 12-meter class telescope, WST, aimed at widefield multi-object and integral field spectroscopy, emphasizing large field of view and high multiplexing.
Contribution
It presents a comprehensive overview of the instrumentation design challenges for WST, including fiber positioning, spectrograph design, and mass production considerations.
Findings
Design solutions for high multiplexing spectroscopy
Strategies for cost-effective mass production
Operational sustainability considerations
Abstract
WST - Widefield Spectroscopic Telescope: We summarise the design challenges of instrumentation for a proposed 12m class Telescope that aims to provide a large (>2.5 square degree) field of view and enable simultaneous Multi-object (> 20,000 objects) and Integral Field spectroscopy (inner 3x3 arcminutes field of view), initially at visible wavelengths. For the MOS mode, instrumentation includes the fiber positioning units, fiber runs and the high (R~40,000) and low (R~3,000 - 4,000) resolution spectrographs. For the MUSE like Integral Field Spectrograph, this includes the relay from the Telescope Focal Plane, the multi-stage splitting and slicing and almost 150 identical spectrographs. We highlight the challenge of mass production at a credible cost and the issues of maintenance and sustainable operation.
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Taxonomy
TopicsAstronomy and Astrophysical Research · Adaptive optics and wavefront sensing · Stellar, planetary, and galactic studies
