Performance of the apache point observatory galactic evolution experiment (APOGEE) high-resolution near-infrared multi-object fiber spectrograph

John C. Wilson; F. Hearty; M. F. Skrutskie; S. R. Majewski; R. Schiavon; D. Eisenstein; J. Gunn; J. Holtzman; D. Nidever; B. Gillespie; D. Weinberg; B. Blank; C. Henderson; S. Smee; R. Barkhouser; A. Harding; S. Hope; G. Fitzgerald; T. Stolberg; J. Arns; M. Nelson; S. Brunner; A. Burton; E. Walker; C. Lam; P. Maseman; J. Barr; F. Leger; L. Carey; N. MacDonald; G. Ebelke; S. Beland; T. Horne; E. Young; G. Rieke; M. Rieke; T. O'Brien; J. Crane; M. Carr; C. Harrison; R. Stoll; M. Vernieri; M. Shetrone; C. Allende-Prieto; J. Johnson; P. Frinchaboy; G. Zasowski; A. Garcia Perez; D. Bizyaev; K. Cunha; V. V. Smith; Sz Meszaros; B. Zhao; M. Hayden; S. D. Chojnowski; B. Andrews; C. Loomis; R. Owen; M. Klaene; J. Brinkmann; F. Stauffer; D. Long; W. Jordan; D. Holder; F. Cope; T. Naugle; B. Pfaffenberger; D. Schlegel; M. Blanton; D. Muna; B. Weaver; S. Snedden; K. Pan; H. Brewington; E. Malanushenko; V. Malanushenko; A. Simmons; D. Oravetz; S. Mahadevan; S. Halverson

doi:10.1117/12.927140

Performance of the apache point observatory galactic evolution experiment (APOGEE) high-resolution near-infrared multi-object fiber spectrograph

John C. Wilson, F. Hearty, M. F. Skrutskie, S. R. Majewski, R. Schiavon, D. Eisenstein, J. Gunn, J. Holtzman, D. Nidever, B. Gillespie, D. Weinberg, B. Blank, C. Henderson, S. Smee, R. Barkhouser, A. Harding, S. Hope, G. Fitzgerald, T. Stolberg, J. ArnsM. Nelson, S. Brunner, A. Burton, E. Walker, C. Lam, P. Maseman, J. Barr, F. Leger, L. Carey, N. MacDonald, G. Ebelke, S. Beland, T. Horne, E. Young, G. Rieke, M. Rieke, T. O'Brien, J. Crane, M. Carr, C. Harrison, R. Stoll, M. Vernieri, M. Shetrone, C. Allende-Prieto, J. Johnson, P. Frinchaboy, G. Zasowski, A. Garcia Perez, D. Bizyaev, K. Cunha, V. V. Smith, Sz Meszaros, B. Zhao, M. Hayden, S. D. Chojnowski, B. Andrews, C. Loomis, R. Owen, M. Klaene, J. Brinkmann, F. Stauffer, D. Long, W. Jordan, D. Holder, F. Cope, T. Naugle, B. Pfaffenberger, D. Schlegel, M. Blanton, D. Muna, B. Weaver, S. Snedden, K. Pan, H. Brewington, E. Malanushenko, V. Malanushenko, A. Simmons, D. Oravetz, S. Mahadevan, S. Halverson

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

65 Scopus citations

Abstract

The Apache Point Observatory Galactic Evolution Experiment (APOGEE) uses a dedicated 300-fiber, narrow-band near-infrared (1.51-1.7 μm), high resolution (R~22,500) spectrograph to survey approximately 100,000 giant stars across the Milky Way. This three-year survey, in operation since late-summer 2011 as part of the Sloan Digital Sky Survey III (SDSS III), will revolutionize our understanding of the kinematical and chemical enrichment histories of all Galactic stellar populations. We present the performance of the instrument from its first year in operation. The instrument is housed in a separate building adjacent to the 2.5-m SDSS telescope and fed light via approximately 45-meter fiber runs from the telescope. The instrument design includes numerous innovations including a gang connector that allows simultaneous connection of all fibers with a single plug to a telescope cartridge that positions the fibers on the sky, numerous places in the fiber train in which focal ratio degradation had to be minimized, a large mosaic-VPH (290 mm x 475 mm elliptically-shaped recorded area), an f/1.4 six-element refractive camera featuring silicon and fused silica elements with diameters as large as 393 mm, three near-infrared detectors mounted in a 1 x 3 mosaic with sub-pixel translation capability, and all of these components housed within a custom, LN₂-cooled, stainless steel vacuum cryostat with dimensions 1.4-m x 2.3-m x 1.3-m.

Original language	English (US)
Title of host publication	Ground-Based and Airborne Instrumentation for Astronomy IV
DOIs	https://doi.org/10.1117/12.927140
State	Published - 2012
Event	Ground-Based and Airborne Instrumentation for Astronomy IV - Amsterdam, Netherlands Duration: Jul 1 2012 → Jul 6 2012

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	8446
ISSN (Print)	0277-786X

Other

Other	Ground-Based and Airborne Instrumentation for Astronomy IV
Country/Territory	Netherlands
City	Amsterdam
Period	7/1/12 → 7/6/12

Keywords

Fiber
Multi-object
Near-Infrared
Spectroscopy
VPH

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.927140

Cite this

Wilson, J. C., Hearty, F., Skrutskie, M. F., Majewski, S. R., Schiavon, R., Eisenstein, D., Gunn, J., Holtzman, J., Nidever, D., Gillespie, B., Weinberg, D., Blank, B., Henderson, C., Smee, S., Barkhouser, R., Harding, A., Hope, S., Fitzgerald, G., Stolberg, T., ... Halverson, S. (2012). Performance of the apache point observatory galactic evolution experiment (APOGEE) high-resolution near-infrared multi-object fiber spectrograph. In Ground-Based and Airborne Instrumentation for Astronomy IV Article 84460H (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 8446). https://doi.org/10.1117/12.927140

Performance of the apache point observatory galactic evolution experiment (APOGEE) high-resolution near-infrared multi-object fiber spectrograph. / Wilson, John C.; Hearty, F.; Skrutskie, M. F. et al.
Ground-Based and Airborne Instrumentation for Astronomy IV. 2012. 84460H (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 8446).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Wilson, JC, Hearty, F, Skrutskie, MF, Majewski, SR, Schiavon, R, Eisenstein, D, Gunn, J, Holtzman, J, Nidever, D, Gillespie, B, Weinberg, D, Blank, B, Henderson, C, Smee, S, Barkhouser, R, Harding, A, Hope, S, Fitzgerald, G, Stolberg, T, Arns, J, Nelson, M, Brunner, S, Burton, A, Walker, E, Lam, C, Maseman, P, Barr, J, Leger, F, Carey, L, MacDonald, N, Ebelke, G, Beland, S, Horne, T, Young, E, Rieke, G , Rieke, M, O'Brien, T, Crane, J, Carr, M, Harrison, C, Stoll, R, Vernieri, M, Shetrone, M, Allende-Prieto, C, Johnson, J, Frinchaboy, P, Zasowski, G, Garcia Perez, A, Bizyaev, D, Cunha, K, Smith, VV, Meszaros, S, Zhao, B, Hayden, M, Chojnowski, SD, Andrews, B, Loomis, C, Owen, R, Klaene, M, Brinkmann, J, Stauffer, F, Long, D, Jordan, W, Holder, D, Cope, F, Naugle, T, Pfaffenberger, B, Schlegel, D, Blanton, M, Muna, D, Weaver, B, Snedden, S, Pan, K, Brewington, H, Malanushenko, E, Malanushenko, V, Simmons, A, Oravetz, D, Mahadevan, S & Halverson, S 2012, Performance of the apache point observatory galactic evolution experiment (APOGEE) high-resolution near-infrared multi-object fiber spectrograph. in Ground-Based and Airborne Instrumentation for Astronomy IV., 84460H, Proceedings of SPIE - The International Society for Optical Engineering, vol. 8446, Ground-Based and Airborne Instrumentation for Astronomy IV, Amsterdam, Netherlands, 7/1/12. https://doi.org/10.1117/12.927140

Wilson JC, Hearty F, Skrutskie MF, Majewski SR, Schiavon R, Eisenstein D et al. Performance of the apache point observatory galactic evolution experiment (APOGEE) high-resolution near-infrared multi-object fiber spectrograph. In Ground-Based and Airborne Instrumentation for Astronomy IV. 2012. 84460H. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.927140

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title = "Performance of the apache point observatory galactic evolution experiment (APOGEE) high-resolution near-infrared multi-object fiber spectrograph",

abstract = "The Apache Point Observatory Galactic Evolution Experiment (APOGEE) uses a dedicated 300-fiber, narrow-band near-infrared (1.51-1.7 μm), high resolution (R~22,500) spectrograph to survey approximately 100,000 giant stars across the Milky Way. This three-year survey, in operation since late-summer 2011 as part of the Sloan Digital Sky Survey III (SDSS III), will revolutionize our understanding of the kinematical and chemical enrichment histories of all Galactic stellar populations. We present the performance of the instrument from its first year in operation. The instrument is housed in a separate building adjacent to the 2.5-m SDSS telescope and fed light via approximately 45-meter fiber runs from the telescope. The instrument design includes numerous innovations including a gang connector that allows simultaneous connection of all fibers with a single plug to a telescope cartridge that positions the fibers on the sky, numerous places in the fiber train in which focal ratio degradation had to be minimized, a large mosaic-VPH (290 mm x 475 mm elliptically-shaped recorded area), an f/1.4 six-element refractive camera featuring silicon and fused silica elements with diameters as large as 393 mm, three near-infrared detectors mounted in a 1 x 3 mosaic with sub-pixel translation capability, and all of these components housed within a custom, LN2-cooled, stainless steel vacuum cryostat with dimensions 1.4-m x 2.3-m x 1.3-m.",

keywords = "Fiber, Multi-object, Near-Infrared, Spectroscopy, VPH",

author = "Wilson, {John C.} and F. Hearty and Skrutskie, {M. F.} and Majewski, {S. R.} and R. Schiavon and D. Eisenstein and J. Gunn and J. Holtzman and D. Nidever and B. Gillespie and D. Weinberg and B. Blank and C. Henderson and S. Smee and R. Barkhouser and A. Harding and S. Hope and G. Fitzgerald and T. Stolberg and J. Arns and M. Nelson and S. Brunner and A. Burton and E. Walker and C. Lam and P. Maseman and J. Barr and F. Leger and L. Carey and N. MacDonald and G. Ebelke and S. Beland and T. Horne and E. Young and G. Rieke and M. Rieke and T. O'Brien and J. Crane and M. Carr and C. Harrison and R. Stoll and M. Vernieri and M. Shetrone and C. Allende-Prieto and J. Johnson and P. Frinchaboy and G. Zasowski and {Garcia Perez}, A. and D. Bizyaev and K. Cunha and Smith, {V. V.} and Sz Meszaros and B. Zhao and M. Hayden and Chojnowski, {S. D.} and B. Andrews and C. Loomis and R. Owen and M. Klaene and J. Brinkmann and F. Stauffer and D. Long and W. Jordan and D. Holder and F. Cope and T. Naugle and B. Pfaffenberger and D. Schlegel and M. Blanton and D. Muna and B. Weaver and S. Snedden and K. Pan and H. Brewington and E. Malanushenko and V. Malanushenko and A. Simmons and D. Oravetz and S. Mahadevan and S. Halverson",

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doi = "10.1117/12.927140",

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series = "Proceedings of SPIE - The International Society for Optical Engineering",

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T1 - Performance of the apache point observatory galactic evolution experiment (APOGEE) high-resolution near-infrared multi-object fiber spectrograph

AU - Wilson, John C.

AU - Hearty, F.

AU - Skrutskie, M. F.

AU - Majewski, S. R.

AU - Schiavon, R.

AU - Eisenstein, D.

AU - Gunn, J.

AU - Holtzman, J.

AU - Nidever, D.

AU - Gillespie, B.

AU - Weinberg, D.

AU - Blank, B.

AU - Henderson, C.

AU - Smee, S.

AU - Barkhouser, R.

AU - Harding, A.

AU - Hope, S.

AU - Fitzgerald, G.

AU - Stolberg, T.

AU - Arns, J.

AU - Nelson, M.

AU - Brunner, S.

AU - Burton, A.

AU - Walker, E.

AU - Lam, C.

AU - Maseman, P.

AU - Barr, J.

AU - Leger, F.

AU - Carey, L.

AU - MacDonald, N.

AU - Ebelke, G.

AU - Beland, S.

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AU - Young, E.

AU - Rieke, G.

AU - Rieke, M.

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AU - Crane, J.

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AU - Harrison, C.

AU - Stoll, R.

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AU - Zasowski, G.

AU - Garcia Perez, A.

AU - Bizyaev, D.

AU - Cunha, K.

AU - Smith, V. V.

AU - Meszaros, Sz

AU - Zhao, B.

AU - Hayden, M.

AU - Chojnowski, S. D.

AU - Andrews, B.

AU - Loomis, C.

AU - Owen, R.

AU - Klaene, M.

AU - Brinkmann, J.

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AU - Long, D.

AU - Jordan, W.

AU - Holder, D.

AU - Cope, F.

AU - Naugle, T.

AU - Pfaffenberger, B.

AU - Schlegel, D.

AU - Blanton, M.

AU - Muna, D.

AU - Weaver, B.

AU - Snedden, S.

AU - Pan, K.

AU - Brewington, H.

AU - Malanushenko, E.

AU - Malanushenko, V.

AU - Simmons, A.

AU - Oravetz, D.

AU - Mahadevan, S.

AU - Halverson, S.

PY - 2012

Y1 - 2012

N2 - The Apache Point Observatory Galactic Evolution Experiment (APOGEE) uses a dedicated 300-fiber, narrow-band near-infrared (1.51-1.7 μm), high resolution (R~22,500) spectrograph to survey approximately 100,000 giant stars across the Milky Way. This three-year survey, in operation since late-summer 2011 as part of the Sloan Digital Sky Survey III (SDSS III), will revolutionize our understanding of the kinematical and chemical enrichment histories of all Galactic stellar populations. We present the performance of the instrument from its first year in operation. The instrument is housed in a separate building adjacent to the 2.5-m SDSS telescope and fed light via approximately 45-meter fiber runs from the telescope. The instrument design includes numerous innovations including a gang connector that allows simultaneous connection of all fibers with a single plug to a telescope cartridge that positions the fibers on the sky, numerous places in the fiber train in which focal ratio degradation had to be minimized, a large mosaic-VPH (290 mm x 475 mm elliptically-shaped recorded area), an f/1.4 six-element refractive camera featuring silicon and fused silica elements with diameters as large as 393 mm, three near-infrared detectors mounted in a 1 x 3 mosaic with sub-pixel translation capability, and all of these components housed within a custom, LN2-cooled, stainless steel vacuum cryostat with dimensions 1.4-m x 2.3-m x 1.3-m.

AB - The Apache Point Observatory Galactic Evolution Experiment (APOGEE) uses a dedicated 300-fiber, narrow-band near-infrared (1.51-1.7 μm), high resolution (R~22,500) spectrograph to survey approximately 100,000 giant stars across the Milky Way. This three-year survey, in operation since late-summer 2011 as part of the Sloan Digital Sky Survey III (SDSS III), will revolutionize our understanding of the kinematical and chemical enrichment histories of all Galactic stellar populations. We present the performance of the instrument from its first year in operation. The instrument is housed in a separate building adjacent to the 2.5-m SDSS telescope and fed light via approximately 45-meter fiber runs from the telescope. The instrument design includes numerous innovations including a gang connector that allows simultaneous connection of all fibers with a single plug to a telescope cartridge that positions the fibers on the sky, numerous places in the fiber train in which focal ratio degradation had to be minimized, a large mosaic-VPH (290 mm x 475 mm elliptically-shaped recorded area), an f/1.4 six-element refractive camera featuring silicon and fused silica elements with diameters as large as 393 mm, three near-infrared detectors mounted in a 1 x 3 mosaic with sub-pixel translation capability, and all of these components housed within a custom, LN2-cooled, stainless steel vacuum cryostat with dimensions 1.4-m x 2.3-m x 1.3-m.

KW - Fiber

KW - Multi-object

KW - Near-Infrared

KW - Spectroscopy

KW - VPH

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DO - 10.1117/12.927140

M3 - Conference contribution

AN - SCOPUS:84871999759

SN - 9780819491473

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Ground-Based and Airborne Instrumentation for Astronomy IV

T2 - Ground-Based and Airborne Instrumentation for Astronomy IV

Y2 - 1 July 2012 through 6 July 2012

ER -

Performance of the apache point observatory galactic evolution experiment (APOGEE) high-resolution near-infrared multi-object fiber spectrograph

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Keywords

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