The DESI Experiment Part II: Instrument Design

Amir Aghamousa,Francisco Prada,Ginevra Favole,K. Honscheid, Timothy A. Hutchinson,Henry D. Heetderks,P. Fosalba,Cristobal Padilla,Nikhil Padmanabhan,Christophe Yèche,Douglas P. Finkbeiner,Yuzo Ishikawa,Theodore Kisner,Jennifer A. Johnson,George F. Smoot,Francisco Valdes, S. Serrano,Richard Massey,Eric Huff,Or Graur,D. Rabinowitz,Pierre-Henri Carton,Carlos Allende Prieto,Ian D. McGreer,Robert C. Nichol,Timothy C. Beers,Abhishek Prakash,Shaun Cole,S. Bailey,Dustin Lang,Richard W. Pogge,Andrew Lambert,Aurélia Secroun,Wojciech A. Hellwing,Timothée Delubac,Debopam Som,Shirley Ho,José Luis Bernal,Violeta Gonzalez-Perez,Michael E. Levi,Graziano Rossi,Sarah Eftekharzadeh,Axel de la Macorra,John Moustakas,Anna Patej, Ryan Staten,Kyle S. Dawson,Yong-Seon Song,Baojiu Li, Xavier Regal, G. Gutierrez,David J. Schlegel, Dara Norman,Andrea Kueter-Young,Terry Gerard,Etienne Burtin,Shadab Alam,S. E. Koposov,Andrew P. Cooper,Jorge Jimenez,Johan Comparat,Anand Raichoor, L. Beaufore, A. Stefanik, A. Roodman,Jean-Gabriel Cuby,Francisco J. Castander,S. Escoffier,Tod R. Lauer,Jorge L. Cervantes-Cota, Shelby Gott,Mehdi Rezaie,Peder Norberg,Alexandre Refregier,Huanyuan Shan,Noble Kennamer,Alistair R. Walker,Chris Bebek,Michele Fumagalli,Claire Poppett,E. S. Rykoff,Otger Ballester, B. Nord,Michael J. Fitzpatrick,Hiranya V. Peiris,Alex Smith,N. MacCrann,Martin White,Denis Gillet,Irena Gershkovich, Ian Heetderks,Hu Zou,Boris T. Gaensicke,Elise Jennings,Andrina Nicola,Salman Habib,Arya Farahi,Hannes Bleuler,R. D. Blum,Nathalie Palanque-Delabrouille,David J. Brooks,Chris Blake,Yutong T. Duan, Yi Zheng,Risa H. Wechsler, Michael Sholl, Robert Besuner,N. Metcalfe, Constance M. Rockosi,David Herrera,Joseph Maria Illa Laguna,Ellie Kitanidis, Daniel Pappalardo,Eric F. Bell,Laleh Makarem,Andreu Font-Ribera,Javier Sanchez, Todd M. Claybaugh,Benjamin A. Weaver, Armin Karcher,Xiaohui Fan,J. García-Bellido, Matthew Evatt,Kazuya Koyama,Jaime E. Forero-Romero,Jeremy L. Tinker,Patrick McDonald,Xu Zhou,Jundan Nie, Luiz Nicolati da Costa,Monica Valluri,A. Ealet, Vanina Ruhlmann-Kleider,Katrin Heitmann,Marc Manera,Huan Lin, N. A. Roe,Jiali Wang,Jean-Paul Kneib,Cristiano G. Sabiu,Benjamin L'Huillier,Richard R. Joyce,Robert Marshall,Cesar Briceno, Mark Derwent, Curtis Weaverdyck, Peter E. Nugent,Ricard Casas,A. M. Meisner,Adam S. Bolton,Jean-Marc Le Goff,Eric V. Linder,Jessica Aguilar,Robert Kehoe,Ho Seong Hwang, William V. Shourt,Daniela Leitner,Minji Oh,Hee-Jong Seo,A. Burden,Nicola Pietro Gentile Fusillo,M. Schubnell,Tianmeng Zhang,Stephen B. H. Kent,J. A. Peacock,Gregory Tarle,Linhua Jiang,Eric Jullo,Lado Samushia,Ming Liang, Auguste Le Van Suu,Michael Schneider,Yuting Wang,Nicholas P. Ross,Robert N. Cahn,Samuel Flender,M. C. Cousinou,Richard G. Kron, Steve Ahlen,Mariana Vargas-Magaña,Rita Tojeiro,A. Ross,Christopher J. Manser,R. Lafever,Zarija Lukić, Samuel Ronayette, David Sprayberry,Changbom Park,E. Gaztanaga,E. Sanchez,Hamsa Padmanabhan, P. Doel,S. Juneau,Gustavo Niz,Paul Martini, Ann Elliott,Carlos S. Frenk,Charles Baltay,Jae Hyeon Lee,Niall Jeffrey,Will J. Percival, Parker Fagrelius, Jeremy McCauley,D. Kirkby, E. Buckley-Geer,Eduardo Rozo,Michael P. Lesser,Beth Reid, Eve Kovacs, James Annis, L. Cardiel-Sas,Milind Naik, Suk Sien Tie,Jeffrey A. Newman,Timothy N. Miller,Raymond G. Carlberg,Sami Kama,Thomas Matheson, Kevin Fanning,M. Crocce,Chang Hee Ree,Sonia Karkar,Gong-Bo Zhao,Jun Ma,Ofer Lahav,Michael Blomqvist,Ray M. Sharples,Jay Farihi,Dianna Jacobs, P. Jelinsky,J. Guy,A. Palmese,Xiyan Peng, Daniel P. Cunningham, Laurent Le Guillou,Knut Olsen,Tamara M. Davis,Govinda Dhungana,Anthony Kremin,Jennifer E. Pollack,Zhimin Zhou,Martin M. Sirk,Adam D. Myers,Stephen Holland,Christophe Magneville,Anze Slosar,Yan-Chuan Cai,David R. Silva,Matthew M. Pieri, Michael L. Lampton,Juan de Vicente,Yaling Zhu, R. Miquel,Florian Beutler, Giuseppe Gallo, Joseph H. Silber,Nicolás G. Busca, E. Fernandez,Joel R. Brownstein,Octavio Valenzuela,Cedric G. Lacey,Thomas O'Brien, Carl T. Coker, Lori E. Allen,K. Reil,Madeline Close, Christophe Balland,Arjun Dey,Sarah R. Loebman, Joseph R. Findlay, Ronald G. Probst,Uros Seljak,T. Giannantonio,Arman Shafieloo,Dragan Huterer, Isabelle Pâris,Martin Landriau,M. Kilbinger,Ying Zu,Zhejie Ding,B. Flaugher,Guillermo Gonzalez-de-Rivera,Alex G. Kim,Daniel J. Eisenstein,Licia Verde, Sandrine Perruchot,Jerry Edelstein,Luzius Kronig,Yu Feng,David H. Weinberg,Qian Yang,Su-Jeong Lee

arXiv: Instrumentation and Methods for Astrophysics(2016)

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摘要
Author(s): Collaboration, DESI; Aghamousa, A; Aguilar, J; Ahlen, S; Alam, S; Allen, LE; Prieto, CA; Annis, J; Bailey, S; Balland, C; Ballester, O; Baltay, C; Beaufore, L; Bebek, C; Beers, TC; Bell, EF; Bernal, JL; Besuner, R; Beutler, F; Blake, C; Bleuler, H; Blomqvist, M; Blum, R; Bolton, AS; Briceno, C; Brooks, D; Brownstein, JR; Buckley-Geer, E; Burden, A; Burtin, E; Busca, NG; Cahn, RN; Cai, Y-C; Cardiel-Sas, L; Carlberg, RG; Carton, P-H; Casas, R; Castander, FJ; Cervantes-Cota, JL; Claybaugh, TM; Close, M; Coker, CT; Cole, S; Comparat, J; Cooper, AP; Cousinou, M-C; Crocce, M; Cuby, J-G; Cunningham, DP; Davis, TM; Dawson, KS; Macorra, ADL; Vicente, JD; Delubac, T; Derwent, M; Dey, A; Dhungana, G; Ding, Z; Doel, P; Duan, YT; Ealet, A; Edelstein, J; Eftekharzadeh, S; Eisenstein, DJ; Elliott, A; Escoffier, S; Evatt, M; Fagrelius, P; Fan, X; Fanning, K; Farahi, A; Farihi, J; Favole, G; Feng, Y; Fernandez, E; Findlay, JR; Finkbeiner, DP; Fitzpatrick, MJ; Flaugher, B; Flender, S; Font-Ribera, A; Forero-Romero, JE; Fosalba, P; Frenk, CS; Fumagalli, M | Abstract: DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of structure through redshift-space distortions with a wide-area galaxy and quasar redshift survey. The DESI instrument is a robotically-actuated, fiber-fed spectrograph capable of taking up to 5,000 simultaneous spectra over a wavelength range from 360 nm to 980 nm. The fibers feed ten three-arm spectrographs with resolution $R= lambda/Deltalambda$ between 2000 and 5500, depending on wavelength. The DESI instrument will be used to conduct a five-year survey designed to cover 14,000 deg$^2$. This powerful instrument will be installed at prime focus on the 4-m Mayall telescope in Kitt Peak, Arizona, along with a new optical corrector, which will provide a three-degree diameter field of view. The DESI collaboration will also deliver a spectroscopic pipeline and data management system to reduce and archive all data for eventual public use.
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