S
Stephen A. Smee
Researcher at Johns Hopkins University
Publications - 96
Citations - 26736
Stephen A. Smee is an academic researcher from Johns Hopkins University. The author has contributed to research in topics: Spectrograph & Telescope. The author has an hindex of 23, co-authored 85 publications receiving 24435 citations. Previous affiliations of Stephen A. Smee include University of Maryland, College Park.
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Journal ArticleDOI
Fourstar: The near-infrared imager for the 6.5 m baade telescope at las campanas observatory
S. E. Persson,D. C. Murphy,Stephen A. Smee,Christoph Birk,Andy Monson,A. Uomoto,E. Koch,Stephen A. Shectman,Robert H. Barkhouser,Joe D. Orndorff,Randy Hammond,Albert Harding,Gregg Scharfstein,D. D. Kelson,Jennifer L. Marshall,Patrick J. McCarthy +15 more
TL;DR: The FourStar Infrared Camera as discussed by the authors is a 4 K × 4 K near-infrared (1.0-2.4 μm) imager built for the Magellan 6.5 m Baade Telescope at Las Campanas Observatory, Chile.
Journal ArticleDOI
MACS?a new high intensity cold neutron spectrometer at NIST
J. A. Rodriguez,J. A. Rodriguez,D M Adler,P.C. Brand,Collin Broholm,Collin Broholm,J.C. Cook,Christoph W. Brocker,Randy Hammond,Z Huang,P Hundertmark,Jeffrey W. Lynn,N. Maliszewskyj,J Moyer,Joe D. Orndorff,D Pierce,T D Pike,Gregg Scharfstein,Stephen A. Smee,Ramon Vilaseca +19 more
TL;DR: In this article, the authors describe a novel cold neutron spectrometer under development at NIST optimized for wave vector resolved spectroscopy with incident energies between 2.1 and 20 meV and energy resolution from 0.05 to 3.0 meV.
Proceedings ArticleDOI
Performance of the Apache Point Observatory Galactic Evolution Experiment (APOGEE) high-resolution near-infrared multi-object fiber spectrograph
John C. Wilson,Frederick R. Hearty,Mike Skrutskie,Steven R. Majewski,Ricardo P. Schiavon,Daniel J. Eisenstein,James E. Gunn,Jon A. Holtzman,David L. Nidever,Bruce Gillespie,David H. Weinberg,Basil Blank,Chuck Henderson,Stephen A. Smee,Robert H. Barkhouser,Albert Harding,Stephen C. Hope,Greg Fitzgerald,T. Stolberg,Jim Arns,Matthew J. Nelson,Sophia Brunner,Adam Burton,E. Walker,Charles R. Lam,Paul Maseman,J. Barr,F. Leger,Larry N. Carey,Nicholas MacDonald,Garrett Ebelke,Stephane Beland,T. Horne,Erick T. Young,George H. Rieke,Marcia J. Rieke,Thomas P. O'Brien,Jeffrey D. Crane,Michael A. Carr,C. Harrison,R. Stoll,M. Vernieri,Matthew Shetrone,Carlos Allende-Prieto,J. A. Johnson,Peter M. Frinchaboy,Gail Zasowski,A. E. García Pérez,D. V. Bizyaev,Katia Cunha,Verne V. Smith,Sz. Meszaros,Bo Zhao,Michael R. Hayden,S. D. Chojnowski,Brett H. Andrews,Craig P. Loomis,Russell Owen,Mark A. Klaene,J. Brinkmann,Fritz Stauffer,Dan Long,Wendell P. Jordan,Diana Holder,Frances Cope,Tracy Naugle,B. Pfaffenberger,David J. Schlegel,M. R. Blanton,Demitri Muna,Benjamin A. Weaver,S. A. Snedden,Kaike Pan,Howard Brewington,Elena Malanushenko,Viktor Malanushenko,A. Simmons,Daniel Oravetz,Suvrath Mahadevan,Samuel Halverson +79 more
TL;DR: The Apache Point Observatory Galactic Evolution Experiment (APOGEE) uses a dedicated 300-fiber, narrow-band near-infrared spectrograph to survey approximately 100,000 giant stars across the Milky Way.
Proceedings ArticleDOI
Prime Focus Spectrograph (PFS) for the Subaru telescope: overview, recent progress, and future perspectives
Naoyuki Tamura,Naruhisa Takato,Atsushi Shimono,Yuki Moritani,Kiyoto Yabe,Yuki Ishizuka,Akitoshi Ueda,Yukiko Kamata,Hrand Aghazarian,Stéphane Arnouts,Gabriel Barban,Robert H. Barkhouser,Renato C. Borges,David F. Braun,Michael A. Carr,Pierre-Yves Chabaud,Yin-Chang Chang,Hsin-Yo Chen,Masashi Chiba,Richard C. Y. Chou,You-Hua Chu,Judith G. Cohen,Rodrigo P. de Almeida,Antonio Cesar de Oliveira,Ligia Souza de Oliveira,Richard Dekany,Kjetil Dohlen,Jesulino Bispo dos Santos,Leandro Henrique dos Santos,Richard S. Ellis,Maximilian Fabricius,Didier Ferrand,Décio Ferreira,Mirek Golebiowski,Jenny E. Greene,Johannes Gross,James E. Gunn,Randolph Hammond,Albert Harding,Murdock Hart,Timothy M. Heckman,Christopher M. Hirata,Paul S. Ho,Stephen C. Hope,Larry E. Hovland,Shu-Fu Hsu,Yen-Shan Hu,Ping-Jie Huang,Marc Jaquet,Yipeng Jing,Jennifer L. Karr,Masahiko Kimura,Matthew E. King,Eiichiro Komatsu,Vincent Le Brun,Olivier Le Fevre,Arnaud Le Fur,David Le Mignant,Hung-Hsu Ling,Craig Loomis,Robert H. Lupton,Fabrice Madec,Peter H. Mao,Lucas Souza Marrara,Claudia Mendes de Oliveira,Yosuke Minowa,Chaz Morantz,Hitoshi Murayama,Graham J. Murray,Youichi Ohyama,Joe D. Orndorff,Sandrine Pascal,Jefferson M. Pereira,Daniel J. Reiley,Martin Reinecke,Andreas Ritter,Mitsuko Roberts,Mark A. Schwochert,Michael Seiffert,Stephen A. Smee,Laerte Sodré,David N. Spergel,Aaron J. Steinkraus,Michael A. Strauss,Christian Surace,Yasushi Suto,Nao Suzuki,John D. Swinbank,Philip J. Tait,Masahiro Takada,Tomonori Tamura,Yoko Tanaka,Laurence Tresse,Orlando Verducci,D. Vibert,Clément Vidal,Shiang-Yu Wang,C.-Y. Wen,Chi-Hung Yan,Naoki Yasuda +99 more
TL;DR: PFS (Prime Focus Spectrograph) as discussed by the authors is a next generation facility instrument on the 8.2-meter Subaru Telescope, which is a very wide-field, massively multiplexed, optical and near-infrared spectrograph.
Journal ArticleDOI
The First Hour of Extragalactic Data of the Sloan Digital Sky Survey Spectroscopic Commissioning: The Coma Cluster
Francisco J. Castander,Robert C. Nichol,Aronne James Merrelli,Aronne James Merrelli,Scott Burles,Scott Burles,Adrian Pope,Adrian Pope,Andrew J. Connolly,Alan Uomoto,James E. Gunn,John E. Anderson,James Annis,Neta A. Bahcall,William N. Boroski,Jon Brinkmann,Larry N. Carey,James H. Crocker,István Csabai,István Csabai,Mamoru Doi,Joshua A. Frieman,Joshua A. Frieman,Masataka Fukugita,Scott D. Friedman,Eric J. Hilton,Robert B. Hindsley,Željko Ivezić,Steve Kent,D. Q. Lamb,R. French Leger,Dan Long,Jon Loveday,Robert H. Lupton,H. T. MacGillivray,Avery Meiksin,Jeffrey A. Munn,M. Newcomb,Sadanori Okamura,Russell Owen,Jeffrey R. Pier,Constance M. Rockosi,David J. Schlegel,Donald P. Schneider,Walter Seigmund,Stephen A. Smee,Yehuda Snir,Larry Starkman,Chris Stoughton,Gyula P. Szokoly,Christopher W. Stubbs,Mark SubbaRao,Alexander S. Szalay,Aniruddha R. Thakar,Christy Tremonti,Patrick Waddell,Brian Yanny,Donald G. York +57 more
TL;DR: In this paper, the first hour of extragalactic spectroscopy taken during these early commissioning stages of the SDSS fiber-fed spectrographs was used for an observation of the Coma cluster of galaxies.