The DESI Experiment Part II: Instrument Design

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, fi...

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Veröffentlicht in:arXiv.org 2016-12
Hauptverfasser: Aguilar, Jessica, Alam, Shadab, Bebek, Chris, Bell, Eric F, Bernal, José Luis, Besuner, Robert, Blake, Chris, Bleuler, Hannes, Bolton, Adam S, Brownstein, Joel R, Burden, Angela, Cardiel-Sas, Laia, Carlberg, Raymond G, Cervantes-Cota, Jorge L, Cooper, Andrew P, M -C Cousinou, Crocce, Martin, Cunningham, Daniel P, Dawson, Kyle S, de la Macorra, Axel, De Vicente, Juan, Doel, Peter, Duan, Yutong T, Ealet, Anne, Eftekharzadeh, Sarah, Elliott, Ann, Fan, Xiaohui, Farihi, Jay, Findlay, Joseph R, Flender, Samuel, ero-Romero, Jaime E, Fumagalli, Michele, Gallo, Giuseppe, Garcia-Bellido, Juan, Gaztanaga, Enrique, Terry, Gerard, Gershkovich, Irena, Gonzalez-Perez, Violeta, Or Graur, Gutierrez, Gaston, Habib, Salman, Heetderks, Ian, Ho, Shirley, Honscheid, Klaus, Hutchinson, Timothy A, Hwang, Ho Seong, Jacobs, Dianna, Niall, Jeffrey, Jennings, Elise, Jimenez, Jorge, Juneau, Stéphanie, Karkar, Sonia, Kehoe, Robert, Noble Kennamer, Kent, Stephen, Kitanidis, Ellie, Kronig, Luzius, Kueter-Young, Andrea, Lambert, Andrew, Laurent Le Guillou, Auguste Le Van Suu, Su-Jeong, Lee, Levi, Michael E, Loebman, Sarah R, Magneville, Christophe, Makarem, Laleh, Manera, Marc, Metcalfe, Nigel, Miquel, Ramon, Naik, Milind, Newman, Jeffrey A, Olsen, Knut A G, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Peiris, Hiranya V, Perruchot, Sandrine, Pogge, Richard, Poppett, Claire, Refregier, Alexandre, Roodman, Aaron, Ross, Nicholas P, Rozo, Eduardo, Sabiu, Cristiano, Lado Samushia, Schneider, Michael, Sharples, Ray, Shourt, William V, Silber, Joseph H, Silva, David R, Som, Debopam, Stefanik, Andy, Valdes, Francisco, Valenzuela, Octavio, Valluri, Monica, Verde, Licia, Yang, Qian, Yeche, Christophe, Zhou, Xu, Zhu, Yaling, Zou, Hu
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creator Aguilar, Jessica
Alam, Shadab
Bebek, Chris
Bell, Eric F
Bernal, José Luis
Besuner, Robert
Blake, Chris
Bleuler, Hannes
Bolton, Adam S
Brownstein, Joel R
Burden, Angela
Cardiel-Sas, Laia
Carlberg, Raymond G
Cervantes-Cota, Jorge L
Cooper, Andrew P
M -C Cousinou
Crocce, Martin
Cunningham, Daniel P
Dawson, Kyle S
de la Macorra, Axel
De Vicente, Juan
Doel, Peter
Duan, Yutong T
Ealet, Anne
Eftekharzadeh, Sarah
Elliott, Ann
Fan, Xiaohui
Farihi, Jay
Findlay, Joseph R
Flender, Samuel
ero-Romero, Jaime E
Fumagalli, Michele
Gallo, Giuseppe
Garcia-Bellido, Juan
Gaztanaga, Enrique
Terry, Gerard
Gershkovich, Irena
Gonzalez-Perez, Violeta
Or Graur
Gutierrez, Gaston
Habib, Salman
Heetderks, Ian
Ho, Shirley
Honscheid, Klaus
Hutchinson, Timothy A
Hwang, Ho Seong
Jacobs, Dianna
Niall, Jeffrey
Jennings, Elise
Jimenez, Jorge
Juneau, Stéphanie
Karkar, Sonia
Kehoe, Robert
Noble Kennamer
Kent, Stephen
Kitanidis, Ellie
Kronig, Luzius
Kueter-Young, Andrea
Lambert, Andrew
Laurent Le Guillou
Auguste Le Van Suu
Su-Jeong, Lee
Levi, Michael E
Loebman, Sarah R
Magneville, Christophe
Makarem, Laleh
Manera, Marc
Metcalfe, Nigel
Miquel, Ramon
Naik, Milind
Newman, Jeffrey A
Olsen, Knut A G
Padmanabhan, Nikhil
Palanque-Delabrouille, Nathalie
Peiris, Hiranya V
Perruchot, Sandrine
Pogge, Richard
Poppett, Claire
Refregier, Alexandre
Roodman, Aaron
Ross, Nicholas P
Rozo, Eduardo
Sabiu, Cristiano
Lado Samushia
Schneider, Michael
Sharples, Ray
Shourt, William V
Silber, Joseph H
Silva, David R
Som, Debopam
Stefanik, Andy
Valdes, Francisco
Valenzuela, Octavio
Valluri, Monica
Verde, Licia
Yang, Qian
Yeche, Christophe
Zhou, Xu
Zhu, Yaling
Zou, Hu
description 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 \(R= \lambda/\Delta\lambda\) 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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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 \(R= \lambda/\Delta\lambda\) 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. 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G</creatorcontrib><creatorcontrib>Padmanabhan, Nikhil</creatorcontrib><creatorcontrib>Palanque-Delabrouille, Nathalie</creatorcontrib><creatorcontrib>Peiris, Hiranya V</creatorcontrib><creatorcontrib>Perruchot, Sandrine</creatorcontrib><creatorcontrib>Pogge, Richard</creatorcontrib><creatorcontrib>Poppett, Claire</creatorcontrib><creatorcontrib>Refregier, Alexandre</creatorcontrib><creatorcontrib>Roodman, Aaron</creatorcontrib><creatorcontrib>Ross, Nicholas P</creatorcontrib><creatorcontrib>Rozo, Eduardo</creatorcontrib><creatorcontrib>Sabiu, Cristiano</creatorcontrib><creatorcontrib>Lado Samushia</creatorcontrib><creatorcontrib>Schneider, Michael</creatorcontrib><creatorcontrib>Sharples, Ray</creatorcontrib><creatorcontrib>Shourt, William V</creatorcontrib><creatorcontrib>Silber, Joseph H</creatorcontrib><creatorcontrib>Silva, David R</creatorcontrib><creatorcontrib>Som, Debopam</creatorcontrib><creatorcontrib>Stefanik, Andy</creatorcontrib><creatorcontrib>Valdes, Francisco</creatorcontrib><creatorcontrib>Valenzuela, Octavio</creatorcontrib><creatorcontrib>Valluri, Monica</creatorcontrib><creatorcontrib>Verde, Licia</creatorcontrib><creatorcontrib>Yang, Qian</creatorcontrib><creatorcontrib>Yeche, Christophe</creatorcontrib><creatorcontrib>Zhou, Xu</creatorcontrib><creatorcontrib>Zhu, Yaling</creatorcontrib><creatorcontrib>Zou, Hu</creatorcontrib><title>The DESI Experiment Part II: Instrument Design</title><title>arXiv.org</title><description>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 \(R= \lambda/\Delta\lambda\) 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.</description><subject>Dark energy</subject><subject>Data management</subject><subject>Field of view</subject><subject>Galaxies</subject><subject>Quasars</subject><subject>Red shift</subject><subject>Spectrographs</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNpjYuA0MjY21LUwMTLiYOAtLs4yMDAwMjM3MjU15mTQC8lIVXBxDfZUcK0oSC3KzE3NK1EISCwqUfD0tFLwzCsuKSoFi7mkFmem5_EwsKYl5hSn8kJpbgZlN9cQZw_dgqL8wtLU4pL4rPzSojygVLyRgYWBmZmJsaWhMXGqAF2GMR4</recordid><startdate>20161213</startdate><enddate>20161213</enddate><creator>Aguilar, Jessica</creator><creator>Alam, 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H</creator><creator>Silva, David R</creator><creator>Som, Debopam</creator><creator>Stefanik, Andy</creator><creator>Valdes, Francisco</creator><creator>Valenzuela, Octavio</creator><creator>Valluri, Monica</creator><creator>Verde, Licia</creator><creator>Yang, Qian</creator><creator>Yeche, Christophe</creator><creator>Zhou, Xu</creator><creator>Zhu, Yaling</creator><creator>Zou, Hu</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20161213</creationdate><title>The DESI Experiment Part II: Instrument Design</title><author>Aguilar, Jessica ; Alam, Shadab ; Bebek, Chris ; Bell, Eric F ; Bernal, José Luis ; Besuner, Robert ; Blake, Chris ; Bleuler, Hannes ; Bolton, Adam S ; Brownstein, Joel R ; Burden, Angela ; Cardiel-Sas, Laia ; Carlberg, Raymond G ; Cervantes-Cota, Jorge L ; Cooper, Andrew P ; M -C Cousinou ; Crocce, Martin ; Cunningham, Daniel P ; Dawson, Kyle S ; de la Macorra, Axel ; De Vicente, Juan ; Doel, Peter ; Duan, Yutong T ; Ealet, Anne ; Eftekharzadeh, Sarah ; Elliott, Ann ; Fan, Xiaohui ; Farihi, Jay ; Findlay, Joseph R ; Flender, Samuel ; ero-Romero, Jaime E ; Fumagalli, Michele ; Gallo, Giuseppe ; Garcia-Bellido, Juan ; Gaztanaga, Enrique ; Terry, Gerard ; Gershkovich, Irena ; Gonzalez-Perez, Violeta ; Or Graur ; Gutierrez, Gaston ; Habib, Salman ; Heetderks, Ian ; Ho, Shirley ; Honscheid, Klaus ; Hutchinson, Timothy A ; Hwang, Ho Seong ; Jacobs, Dianna ; Niall, Jeffrey ; Jennings, Elise ; Jimenez, Jorge ; Juneau, Stéphanie ; Karkar, Sonia ; Kehoe, Robert ; Noble Kennamer ; Kent, Stephen ; Kitanidis, Ellie ; Kronig, Luzius ; Kueter-Young, Andrea ; Lambert, Andrew ; Laurent Le Guillou ; Auguste Le Van Suu ; Su-Jeong, Lee ; Levi, Michael E ; Loebman, Sarah R ; Magneville, Christophe ; Makarem, Laleh ; Manera, Marc ; Metcalfe, Nigel ; Miquel, Ramon ; Naik, Milind ; Newman, Jeffrey A ; Olsen, Knut A G ; Padmanabhan, Nikhil ; Palanque-Delabrouille, Nathalie ; Peiris, Hiranya V ; Perruchot, Sandrine ; Pogge, Richard ; Poppett, Claire ; Refregier, Alexandre ; Roodman, Aaron ; Ross, Nicholas P ; Rozo, Eduardo ; Sabiu, Cristiano ; Lado Samushia ; Schneider, Michael ; Sharples, Ray ; Shourt, William V ; Silber, Joseph H ; Silva, David R ; Som, Debopam ; Stefanik, Andy ; Valdes, Francisco ; Valenzuela, Octavio ; Valluri, Monica ; Verde, Licia ; Yang, Qian ; Yeche, Christophe ; Zhou, Xu ; Zhu, Yaling ; Zou, Hu</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20806643913</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Dark energy</topic><topic>Data management</topic><topic>Field of view</topic><topic>Galaxies</topic><topic>Quasars</topic><topic>Red shift</topic><topic>Spectrographs</topic><toplevel>online_resources</toplevel><creatorcontrib>Aguilar, Jessica</creatorcontrib><creatorcontrib>Alam, Shadab</creatorcontrib><creatorcontrib>Bebek, Chris</creatorcontrib><creatorcontrib>Bell, Eric F</creatorcontrib><creatorcontrib>Bernal, José Luis</creatorcontrib><creatorcontrib>Besuner, Robert</creatorcontrib><creatorcontrib>Blake, Chris</creatorcontrib><creatorcontrib>Bleuler, Hannes</creatorcontrib><creatorcontrib>Bolton, Adam S</creatorcontrib><creatorcontrib>Brownstein, Joel R</creatorcontrib><creatorcontrib>Burden, Angela</creatorcontrib><creatorcontrib>Cardiel-Sas, 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Michele</creatorcontrib><creatorcontrib>Gallo, Giuseppe</creatorcontrib><creatorcontrib>Garcia-Bellido, Juan</creatorcontrib><creatorcontrib>Gaztanaga, Enrique</creatorcontrib><creatorcontrib>Terry, Gerard</creatorcontrib><creatorcontrib>Gershkovich, Irena</creatorcontrib><creatorcontrib>Gonzalez-Perez, Violeta</creatorcontrib><creatorcontrib>Or Graur</creatorcontrib><creatorcontrib>Gutierrez, Gaston</creatorcontrib><creatorcontrib>Habib, Salman</creatorcontrib><creatorcontrib>Heetderks, Ian</creatorcontrib><creatorcontrib>Ho, Shirley</creatorcontrib><creatorcontrib>Honscheid, Klaus</creatorcontrib><creatorcontrib>Hutchinson, Timothy A</creatorcontrib><creatorcontrib>Hwang, Ho Seong</creatorcontrib><creatorcontrib>Jacobs, Dianna</creatorcontrib><creatorcontrib>Niall, Jeffrey</creatorcontrib><creatorcontrib>Jennings, Elise</creatorcontrib><creatorcontrib>Jimenez, Jorge</creatorcontrib><creatorcontrib>Juneau, Stéphanie</creatorcontrib><creatorcontrib>Karkar, Sonia</creatorcontrib><creatorcontrib>Kehoe, Robert</creatorcontrib><creatorcontrib>Noble Kennamer</creatorcontrib><creatorcontrib>Kent, Stephen</creatorcontrib><creatorcontrib>Kitanidis, Ellie</creatorcontrib><creatorcontrib>Kronig, Luzius</creatorcontrib><creatorcontrib>Kueter-Young, Andrea</creatorcontrib><creatorcontrib>Lambert, Andrew</creatorcontrib><creatorcontrib>Laurent Le Guillou</creatorcontrib><creatorcontrib>Auguste Le Van Suu</creatorcontrib><creatorcontrib>Su-Jeong, Lee</creatorcontrib><creatorcontrib>Levi, Michael E</creatorcontrib><creatorcontrib>Loebman, Sarah R</creatorcontrib><creatorcontrib>Magneville, Christophe</creatorcontrib><creatorcontrib>Makarem, Laleh</creatorcontrib><creatorcontrib>Manera, Marc</creatorcontrib><creatorcontrib>Metcalfe, Nigel</creatorcontrib><creatorcontrib>Miquel, Ramon</creatorcontrib><creatorcontrib>Naik, Milind</creatorcontrib><creatorcontrib>Newman, Jeffrey A</creatorcontrib><creatorcontrib>Olsen, Knut A G</creatorcontrib><creatorcontrib>Padmanabhan, Nikhil</creatorcontrib><creatorcontrib>Palanque-Delabrouille, Nathalie</creatorcontrib><creatorcontrib>Peiris, Hiranya V</creatorcontrib><creatorcontrib>Perruchot, Sandrine</creatorcontrib><creatorcontrib>Pogge, Richard</creatorcontrib><creatorcontrib>Poppett, Claire</creatorcontrib><creatorcontrib>Refregier, Alexandre</creatorcontrib><creatorcontrib>Roodman, Aaron</creatorcontrib><creatorcontrib>Ross, Nicholas P</creatorcontrib><creatorcontrib>Rozo, Eduardo</creatorcontrib><creatorcontrib>Sabiu, Cristiano</creatorcontrib><creatorcontrib>Lado Samushia</creatorcontrib><creatorcontrib>Schneider, Michael</creatorcontrib><creatorcontrib>Sharples, Ray</creatorcontrib><creatorcontrib>Shourt, William V</creatorcontrib><creatorcontrib>Silber, Joseph H</creatorcontrib><creatorcontrib>Silva, David R</creatorcontrib><creatorcontrib>Som, Debopam</creatorcontrib><creatorcontrib>Stefanik, Andy</creatorcontrib><creatorcontrib>Valdes, Francisco</creatorcontrib><creatorcontrib>Valenzuela, Octavio</creatorcontrib><creatorcontrib>Valluri, Monica</creatorcontrib><creatorcontrib>Verde, Licia</creatorcontrib><creatorcontrib>Yang, Qian</creatorcontrib><creatorcontrib>Yeche, Christophe</creatorcontrib><creatorcontrib>Zhou, Xu</creatorcontrib><creatorcontrib>Zhu, Yaling</creatorcontrib><creatorcontrib>Zou, Hu</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Aguilar, Jessica</au><au>Alam, Shadab</au><au>Bebek, Chris</au><au>Bell, Eric F</au><au>Bernal, José Luis</au><au>Besuner, Robert</au><au>Blake, Chris</au><au>Bleuler, Hannes</au><au>Bolton, Adam S</au><au>Brownstein, Joel R</au><au>Burden, Angela</au><au>Cardiel-Sas, Laia</au><au>Carlberg, Raymond G</au><au>Cervantes-Cota, Jorge L</au><au>Cooper, Andrew P</au><au>M -C Cousinou</au><au>Crocce, Martin</au><au>Cunningham, Daniel P</au><au>Dawson, Kyle S</au><au>de la Macorra, Axel</au><au>De Vicente, Juan</au><au>Doel, Peter</au><au>Duan, Yutong T</au><au>Ealet, Anne</au><au>Eftekharzadeh, Sarah</au><au>Elliott, Ann</au><au>Fan, Xiaohui</au><au>Farihi, Jay</au><au>Findlay, Joseph R</au><au>Flender, Samuel</au><au>ero-Romero, Jaime E</au><au>Fumagalli, Michele</au><au>Gallo, Giuseppe</au><au>Garcia-Bellido, Juan</au><au>Gaztanaga, Enrique</au><au>Terry, Gerard</au><au>Gershkovich, Irena</au><au>Gonzalez-Perez, Violeta</au><au>Or Graur</au><au>Gutierrez, Gaston</au><au>Habib, Salman</au><au>Heetderks, Ian</au><au>Ho, Shirley</au><au>Honscheid, Klaus</au><au>Hutchinson, Timothy A</au><au>Hwang, Ho Seong</au><au>Jacobs, Dianna</au><au>Niall, Jeffrey</au><au>Jennings, Elise</au><au>Jimenez, Jorge</au><au>Juneau, Stéphanie</au><au>Karkar, Sonia</au><au>Kehoe, Robert</au><au>Noble Kennamer</au><au>Kent, Stephen</au><au>Kitanidis, Ellie</au><au>Kronig, Luzius</au><au>Kueter-Young, Andrea</au><au>Lambert, Andrew</au><au>Laurent Le Guillou</au><au>Auguste Le Van Suu</au><au>Su-Jeong, Lee</au><au>Levi, Michael E</au><au>Loebman, Sarah R</au><au>Magneville, Christophe</au><au>Makarem, Laleh</au><au>Manera, Marc</au><au>Metcalfe, Nigel</au><au>Miquel, Ramon</au><au>Naik, Milind</au><au>Newman, Jeffrey A</au><au>Olsen, Knut A G</au><au>Padmanabhan, Nikhil</au><au>Palanque-Delabrouille, Nathalie</au><au>Peiris, Hiranya V</au><au>Perruchot, Sandrine</au><au>Pogge, Richard</au><au>Poppett, Claire</au><au>Refregier, Alexandre</au><au>Roodman, Aaron</au><au>Ross, Nicholas P</au><au>Rozo, Eduardo</au><au>Sabiu, Cristiano</au><au>Lado Samushia</au><au>Schneider, Michael</au><au>Sharples, Ray</au><au>Shourt, William V</au><au>Silber, Joseph H</au><au>Silva, David R</au><au>Som, Debopam</au><au>Stefanik, Andy</au><au>Valdes, Francisco</au><au>Valenzuela, Octavio</au><au>Valluri, Monica</au><au>Verde, Licia</au><au>Yang, Qian</au><au>Yeche, Christophe</au><au>Zhou, Xu</au><au>Zhu, Yaling</au><au>Zou, Hu</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>The DESI Experiment Part II: Instrument Design</atitle><jtitle>arXiv.org</jtitle><date>2016-12-13</date><risdate>2016</risdate><eissn>2331-8422</eissn><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 \(R= \lambda/\Delta\lambda\) 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.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record>
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subjects Dark energy
Data management
Field of view
Galaxies
Quasars
Red shift
Spectrographs
title The DESI Experiment Part II: Instrument Design
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