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The Robotic Multiobject Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI)

  • Authors: 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

Joseph Harry Silber et al 2023 The Astronomical Journal 165 .

  • Provider: AAS Journals

Caption: Figure 15.

Each as-built petal was robotically surveyed and aligned such that fiber tips, fiducials, and cameras, when installed, would land in focus on DESI's nominal aspheric focal surface. The upper-left and lower-right photos show the FPR and petals being surveyed in a CMM at LBNL. The two photos at the lower left show the GFA camera mount plate on a petal, which is adjusted by shimming at its three mount screws. At the upper right, a stack of two gauge blocks and an aluminum retention/contact pad are seen at the corner of a petal. Each petal has two of these, which contact the FPR, and give us both stiff mounting and fine tilt adjustment. Not shown in these photos are two additional adjustment features of the petals: these are captive shim stacks at (1) the outer radius, to set the focal position, and (2) at the inner radius Figure 11, to equalize the petals with respect to each other at their tips. Over the set of all 12 petals (10 installed plus two spares), we achieved 12 μm rms, 33 μm max error in our alignment.

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