Overview of the Fiber System for the Dark Energy Spectroscopic Instrument

Poppett, Claire; Tyas, Luke; Aguilar, J.; Bebek, Christopher; Bramall, D.; Claybaugh, T.; Edelstein, J.; Fagrelius, P.; Heetderks, H.; Jelinsky, P.; Jelinsky, S.; Lafever, Robin; Lambert, A.; Lampton, M.; Levi, Michael E.; Martini, P.; Rockosi, C.; Schmoll, J.; Sharples, Ray M.; Sirk, Martin; Wishnow, Edward; Yu, Jiaxi; Ahlen, S.; Bault, A.; BenZvi, S.; Brooks, D.; Cole, S.; de la Macorra, A.; Dey, Arjun; Doel, P.; Fanning, K.; Font-Ribera, A.; Forero-Romero, J. E.; Gaztañaga, E.; Gontcho A Gontcho, S.; Gonzalez-Morales, A. X.; Hahn, C.; Honscheid, K.; Jimenez, J.; Juneau, S.; Kirkby, D.; Kremin, A.; Landriau, M.; Le Guillou, L.; Manera, M.; Meisner, A.; Miquel, R.; Moustakas, J.; Mueller, E.; Muñoz-Gutiérrez, A.; Myers, A. D.; Nie, J.; Niz, G.; Palanque-Delabrouille, N.; Percival, W. J.; Prada, F.; Rabinowitz, D.; Rezaie, M.; Rossi, G.; Sanchez, E.; Schlafly, Edward F.; Schlegel, D.; Schubnell, M.; Seo, H.; Sprayberry, D.; Tarlé, G.; Vargas-Magaña, M.; Weaver, B. A.; Zhou, R.

Abstract

The Dark Energy Spectroscopic Instrument (DESI) is a revolutionary instrument designed for precise measurements of cosmic distances and the investigation of dark energy. DESI utilizes 5000 optical fibers to simultaneously measure the spectra of distant objects and aims to measure 40 million galaxies and quasars in a 5 yr survey. One of the critical challenges to DESI’s success was ensuring that the fiber system was not only highly efficient but also delivered a highly stable beam enabling more reliable sky subtraction for measurements of faint objects. We achieved this stability by minimizing the stress on the fiber system during the manufacture and operation of the telescope and fiber positioning robots. We installed the DESI fiber system on the 4 m Mayall telescope with ≥99% of fibers intact, and the instrument has delivered superb optical performance throughout the initial years of the DESI survey, including ≥90% average throughput when injected with a focal ratio of ∼f/3.9 as delivered by the primary focus corrector, excluding fiber absorption losses. The design of DESI required multiple innovations to achieve these requirements, such as cleaved fibers bonded with a UV-curing epoxy to glass ferrules in the focal plane and fusion splicing instead of physical connectors. In this paper, we describe the development, delivery, and installation of the fiber system, the innovations that made the state-of-the-art performance possible, and the key lessons learned that could benefit future projects.

Citation

Poppett, C., Tyas, L., Aguilar, J., Bebek, C., Bramall, D., Claybaugh, T., Edelstein, J., Fagrelius, P., Heetderks, H., Jelinsky, P., Jelinsky, S., Lafever, R., Lambert, A., Lampton, M., Levi, M. E., Martini, P., Rockosi, C., Schmoll, J., Sharples, R. M., Sirk, M., …Zhou, R. (2024). Overview of the Fiber System for the Dark Energy Spectroscopic Instrument. Astronomical Journal, 168(6), Article 245. https://doi.org/10.3847/1538-3881/ad76a4

• Journal Article Type: Article
• Acceptance Date: Sep 1, 2024
• Online Publication Date: Nov 8, 2024
• Publication Date: Dec 1, 2024
• Deposit Date: Nov 13, 2024
• Publicly Available Date: Nov 13, 2024
• Journal: The Astronomical Journal
• Print ISSN: 0004-6256
• Electronic ISSN: 1538-3881
• Publisher: IOP Publishing
• Peer Reviewed: Peer Reviewed
• Volume: 168
• Issue: 6
• Article Number: 245
• DOI: https://doi.org/10.3847/1538-3881/ad76a4
• Keywords: Galaxy spectroscopy, Cosmological evolution, Astronomical instrumentation
• Public URL: https://durham-repository.worktribe.com/output/3090438