학술논문
The Robotic Multiobject Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI)
Document Type
article
Author
Joseph Harry Silber; Parker Fagrelius; Kevin Fanning; Michael Schubnell; Jessica Nicole Aguilar; Steven Ahlen; Jon Ameel; Otger Ballester; Charles Baltay; Chris Bebek; Dominic Benton Beard; Robert Besuner; Laia Cardiel-Sas; Ricard Casas; Francisco Javier Castander; Todd Claybaugh; Carl Dobson; Yutong Duan; Patrick Dunlop; Jerry Edelstein; William T. Emmet; Ann Elliott; Matthew Evatt; Irena Gershkovich; Julien Guy; Stu Harris; Henry Heetderks; Ian Heetderks; Klaus Honscheid; Jose Maria Illa; Patrick Jelinsky; Sharon R. Jelinsky; Jorge Jimenez; Armin Karcher; Stephen Kent; David Kirkby; Jean-Paul Kneib; Andrew Lambert; Mike Lampton; Daniela Leitner; Michael Levi; Jeremy McCauley; Aaron Meisner; Timothy N. Miller; Ramon Miquel; Juliá Mundet; Claire Poppett; David Rabinowitz; Kevin Reil; David Roman; David Schlegel; Santiago Serrano; William Van Shourt; David Sprayberry; Gregory Tarlé; Suk Sien Tie; Curtis Weaverdyck; Kai Zhang; Marco Azzaro; Stephen Bailey; Santiago Becerril; Tami Blackwell; Mohamed Bouri; David Brooks; Elizabeth Buckley-Geer; Jose Peñate Castro; Mark Derwent; Arjun Dey; Govinda Dhungana; Peter Doel; Daniel J. Eisenstein; Nasib Fahim; Juan Garcia-Bellido; Enrique Gaztañaga; Satya Gontcho A Gontcho; Gaston Gutierrez; Philipp Hörler; Robert Kehoe; Theodore Kisner; Anthony Kremin; Luzius Kronig; Martin Landriau; Laurent Le Guillou; Paul Martini; John Moustakas; Nathalie Palanque-Delabrouille; Xiyan Peng; Will Percival; Francisco Prada; Carlos Allende Prieto; Guillermo Gonzalez de Rivera; Eusebio Sanchez; Justo Sanchez; Ray Sharples; Marcelle Soares-Santos; Edward Schlafly; Benjamin Alan Weaver; Zhimin Zhou; Yaling Zhu; Hu Zou; (DESI Collaboration)
Source
The Astronomical Journal, Vol 165, Iss 1, p 9 (2022)
Subject
Language
English
ISSN
1538-3881
Abstract
A system of 5020 robotic fiber positioners was installed in 2019 on the Mayall Telescope, at Kitt Peak National Observatory. The robots automatically retarget their optical fibers every 10–20 minutes, each to a precision of several microns, with a reconfiguration time of fewer than 2 minutes. Over the next 5 yr, they will enable the newly constructed Dark Energy Spectroscopic Instrument (DESI) to measure the spectra of 35 million galaxies and quasars. DESI will produce the largest 3D map of the universe to date and measure the expansion history of the cosmos. In addition to the 5020 robotic positioners and optical fibers, DESI’s Focal Plane System includes six guide cameras, four wave front cameras, 123 fiducial point sources, and a metrology camera mounted at the primary mirror. The system also includes associated structural, thermal, and electrical systems. In all, it contains over 675,000 individual parts. We discuss the design, construction, quality control, and integration of all these components. We include a summary of the key requirements, the review and acceptance process, on-sky validations of requirements, and lessons learned for future multiobject, fiber-fed spectrographs.