4.6 Article

THE BOSS Lyα FOREST SAMPLE FROM SDSS DATA RELEASE 9

Journal

ASTRONOMICAL JOURNAL
Volume 145, Issue 3, Pages -

Publisher

IOP Publishing Ltd
DOI: 10.1088/0004-6256/145/3/69

Keywords

intergalactic medium; methods: data analysis; quasars: absorption lines; quasars: emission lines

Funding

  1. European Union [PIIF-GA-2011-301665]
  2. Alfred P. Sloan Foundation
  3. National Science Foundation
  4. U.S. Department of Energy Office of Science
  5. University of Arizona
  6. Brazilian Participation Group
  7. Brookhaven National Laboratory
  8. University of Cambridge
  9. Carnegie Mellon University
  10. University of Florida
  11. French Participation Group
  12. German Participation Group
  13. Harvard University
  14. Instituto de Astrofisica de Canarias
  15. Michigan State/Notre Dame/JINA Participation Group
  16. Johns Hopkins University
  17. Lawrence Berkeley National Laboratory
  18. Max Planck Institute for Astrophysics
  19. Max Planck Institute for Extraterrestrial Physics
  20. New Mexico State University
  21. New York University
  22. Ohio State University
  23. Pennsylvania State University
  24. University of Portsmouth
  25. Princeton University
  26. Spanish Participation Group, University of Tokyo
  27. University of Utah
  28. Vanderbilt University
  29. University of Virginia
  30. University of Washington
  31. Yale University
  32. Direct For Mathematical & Physical Scien
  33. Division Of Astronomical Sciences [1109730] Funding Source: National Science Foundation
  34. Division Of Astronomical Sciences
  35. Direct For Mathematical & Physical Scien [1202963] Funding Source: National Science Foundation
  36. ICREA Funding Source: Custom

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We present the BOSS Lyman-alpha (Ly alpha) Forest Sample from SDSS Data Release 9, comprising 54,468 quasar spectra with z(qso) > 2.15 suitable for Ly alpha forest analysis. This data set probes the intergalactic medium with absorption redshifts 2.0 < z alpha < 5.7 over an area of 3275 deg(2), and encompasses an approximate comoving volume of 20 h(-3) Gpc(3). With each spectrum, we have included several products designed to aid in Ly alpha forest analysis: improved sky masks that flag pixels where data may be unreliable, corrections for known biases in the pipeline estimated noise, masks for the cores of damped Ly alpha systems and corrections for their wings, and estimates of the unabsorbed continua so that the observed flux can be converted to a fractional transmission. The continua are derived using a principal component fit to the quasar spectrum redward of rest-frame Ly alpha (lambda > 1216 angstrom), extrapolated into the forest region and normalized by a linear function to fit the expected evolution of the Ly alpha forest mean flux. The estimated continuum errors are less than or similar to 5% rms. We also discuss possible systematics arising from uncertain spectrophotometry and artifacts in the flux calibration; global corrections for the latter are provided. Our sample provides a convenient starting point for users to analyze clustering in BOSS Ly alpha forest data, and it provides a fiducial data set that can be used to compare results from different analyses of baryon acoustic oscillations in the Ly alpha forest. The full data set is available from the SDSS-III DR9 Web site.

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