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The Baryon Oscilliation Spectroscopic Survey of SDSS-II

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  • Kyle S. Dawson
  • David J. Schlegel
  • Christopher P. Ahn
  • Scott F. Anderson
  • Eric Aubourg
  • Stephen Bailey
  • Robert H. Barkhouser
  • Alessandra Beifiori
  • Andreas A. Berlind
  • Vaishali Bhardwaj
  • Dmitry Bizyaev
  • Cullen H. Blake
  • Michael R. Blanton
  • Michael Blomqvist
  • Adam S. Bolton
  • Arnaud Borde
  • Jo Bovy
  • W. N. Brandt
  • Howard Brewington
  • Jon Brinkmann
  • Peter J. Brown
  • Joel R. Brownstein
  • Kevin Bundy
  • N. G. Busca
  • William Carithers
  • Aurelio R. Carnero
  • Michael A. Carr
  • Yanmei Chen
  • Johan Comparat
  • Natalia Connolly
  • Frances Cope
  • Rupert A. C. Croft
  • Antonio J. Cuesta
  • Luiz N. da Costa
  • James R. A. Davenport
  • Timothee Delubac
  • Roland de Putter
  • Saurav Dhital
  • Anne Ealet
  • Garrett L. Ebelke
  • Daniel J. Eisenstein
  • S. Escoffier
  • Xiaohui Fan
  • N. Filiz Ak
  • Hayley Finley
  • Andreu Font-Ribera
  • R. Genova-Santos
  • James E. Gunn
  • Hong Guo
  • Daryl Haggard
  • Patrick B. Hall
  • Jean-Christophe Hamilton
  • Ben Harris
  • David W. Harris
  • Shirley Ho
  • David W. Hogg
  • Diana Holder
  • Klaus Honscheid
  • Joe Huehnerhoff
  • Beatrice Jordan
  • Wendell P. Jordan
  • Guinevere Kauffmann
  • Eyal A. Kazin
  • David Kirkby
  • Mark A. Klaene
  • Jean-Paul Kneib
  • Jean-Marc Le Goff
  • Khee-Gan Lee
  • Daniel C. Long
  • Craig P. Loomis
  • Britt Lundgren
  • Robert H. Lupton
  • Marcio A. G. Maia
  • Martin Makler
  • Elena Malanushenko
  • Viktor Malanushenko
  • Rachel Mandelbaum
  • Marc Manera
  • Daniel Margala
  • Karen L. Masters
  • Cameron K. McBride
  • Patrick McDonald
  • Ian D. McGreer
  • Richard G. McMahon
  • Olga Mena
  • Jordi Miralda-Escude
  • Antonio D. Montero-Dorta
  • Francesco Montesano
  • Demitri Muna
  • Adam D. Myers
  • Tracy Naugle
  • Pasquier Noterdaeme
  • Sebastian E. Nuza
  • Matthew D. Olmstead
  • Audrey Oravetz
  • Daniel J. Oravetz
  • Russell Owen
  • Nikhil Padmanabhan
  • Nathalie Palanque-Delabrouille
  • Kaike Pan
  • John K. Parejko
  • Isabelle Paris
  • Will J. Percival
  • Ismael Perez-Fournon
  • Ignasi Perez-Rafols
  • Patrick Petitjean
  • Robert Pfaffenberger
  • Janine Pforr
  • Matthew M. Pieri
  • Francisco Prada
  • Adrian M. Price-Whelan
  • M. Jordan Raddick
  • Rafael Rebolo
  • James Rich
  • Gordon T. Richards
  • Constance M. Rockosi
  • Natalie A. Roe
  • Nicholas P. Ross
  • Graziano Rossi
  • J. A. Rubino-Martin
  • Ariel G. Sanchez
  • Conor Sayres
  • Sarah J. Schmidt
  • Donald P. Schneider
  • C. G. Scoccola
  • Hee-Jong Seo
  • Alaina Shelden
  • Erin Sheldon
  • Yue Shen
  • Yiping Shu
  • Anze Slosar
  • Stephen A. Smee
  • Stephanie A. Snedden
  • Fritz Stauffer
  • Oliver Steele
  • Michael A. Strauss
  • Alina Streblyanska
  • Nao Suzuki
  • Molly E. C. Swanson
  • Tomer Tal
  • Masayuki Tanaka
  • Jeremy L. Tinker
  • Rita Tojeiro
  • Christy A. Tremonti
  • M. Vargas Magana
  • Licia Verde
  • Matteo Viel
  • David A. Wake
  • Mike Watson
  • Benjamin A. Weaver
  • David H. Weinberg
  • Benjamin J. Weiner
  • Andrew A. West
  • Martin White
  • W. M. Wood-Vasey
  • Christophe Yeche
  • Idit Zehavi
  • Gong-Bo Zhao
  • Zheng Zheng
The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger volume than the combined efforts of all previous spectroscopic surveys of large-scale structure. BOSS uses 1.5 million luminous galaxies as faint as i = 19.9 over 10,000 deg2 to measure BAO to redshifts z < 0.7. Observations of neutral hydrogen in the Lyα forest in more than 150,000 quasar spectra (g < 22) will constrain BAO over the redshift range 2.15 < z < 3.5. Early results from BOSS include the first detection of the large-scale three-dimensional clustering of the Lyα forest and a strong detection from the Data Release 9 data set of the BAO in the clustering of massive galaxies at an effective redshift z = 0.57. We project that BOSS will yield measurements of the angular diameter distance dA to an accuracy of 1.0% at redshifts z = 0.3 and z = 0.57 and measurements of H(z) to 1.8% and 1.7% at the same redshifts. Forecasts for Lyα forest constraints predict a measurement of an overall dilation factor that scales the highly degenerate DA (z) and H –1(z) parameters to an accuracy of 1.9% at z ~ 2.5 when the survey is complete. Here, we provide an overview of the selection of spectroscopic targets, planning of observations, and analysis of data and data quality of BOSS.
Original languageEnglish
Article number10
Pages (from-to)10
JournalThe Astronomical Journal
Volume145
Issue number1
Early online date6 Dec 2012
DOIs
Publication statusPublished - Jan 2013

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