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Wide-Field Multi-Object Spectrograph

(WFMOS)
(proposed instrument to detect baryon acoustic oscillations)

The Wide-Field Multi-Object Spectrograph (WFMOS) was a proposed instrument for research in Cosmology. It aimed to identify many distant galaxies with information about their positions, under the assumption that this would show a tendency for galaxies to be found 150 Parsecs distant from each other, a signature of Baryon Acoustic Oscillations.

The WFMOS was intended for one of the Gemini Observatory telescopes and later the Subaru Telescope and a new plan (the Subaru PFS Spectrograph) is aimed at its niche.


(instrument,cosmology,spectrograph,plan,past)
https://www.noao.edu/meetings/subaru/Session-1/Colless.pdf
https://www.naoj.org/Projects/wfmos2008/program/Talks/Jensen.pdf

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