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25,000 optical fiber positioning robots for next-generation cosmology

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arxiv 2212.07908 v1 pith:YOZHBKVP submitted 2022-12-15 astro-ph.IM astro-ph.GA

classification astro-ph.IMastro-ph.GA
keywords cosmologyrobotsdarkenergyfibergenerationinstrumentsnext
verification ladder T0 review T1 audit T2 compute T3 formal
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Massively parallel multi-object spectrographs are on the leading edge of cosmology instrumentation. The highly successful Dark Energy Spectroscopic Instrument (DESI) which begun survey operations in May 2021, for example, has 5,000 robotically-actuated multimode fibers, which deliver light from thousands of individual galaxies and quasars simultaneously to an array of high-resolution spectrographs off-telescope. The redshifts are individually measured, thus providing 3D maps of the Universe in unprecedented detail, and enabling precise measurement of dark energy expansion and other key cosmological parameters. Here we present new work in the design and prototyping of the next generation of fiber-positioning robots. At 6.2 mm center-to-center pitch, with 1-2 um positioning precision, and in a scalable form factor, these devices will enable the next generation of cosmology instruments, scaling up to instruments with 10,000 to 25,000 fiber robots.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Linear motion (R-FLEX) for minature 6.2 mm pitch optical fiber position robots with polar (R-theta) kinematics

    astro-ph.IM 2026-07 conditional novelty 6.0 of 10

    A compact flexure-based radial positioner for 6.2 mm-pitch fiber robots achieves <4 µm RMS corrected accuracy, 0.092° max tilt, 42 µm defocus, and >400,000-target durability in two prototypes.

  2. Prototyping of 6.2-mm-Pitch Fiber Positioner Modules for Stage-V Telescope Instrumentation

    astro-ph.IM 2025-08 conditional novelty 5.0 of 10

    Prototyping and quantitative evaluation of 6.2-mm-pitch alpha-beta fiber positioner modules showing encouraging positioning accuracy and low fiber tilt for Stage-V spectroscopic surveys.

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