Published March 2013 | Version v1
Journal article

THE BOSS Lyα FOREST SAMPLE FROM SDSS DATA RELEASE 9

  • 1. Max Planck Institute for Astronomy, Königstuhl 17, D-69115 Heidelberg (Germany)
  • 2. Lawrence Berkeley National Lab, 1 Cyclotron Rd, Berkeley, CA 94720 (United States)
  • 3. Department of Physics, Carnegie Mellon University, 5000 Forbes Ave, Pittsburgh, PA 15213 (United States)
  • 4. Department of Physics and Astronomy, University of Utah, 115 S 1400 E, Salt Lake City, UT 84112 (United States)
  • 5. Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States)
  • 6. Department of Astronomy, University of Wisconsin, 475 North Charter Street, Madison, WI 53706 (United States)
  • 7. CEA, Centre de Saclay, Irfu/SPP, F-91191 Gif-sur-Yvette (France)
  • 8. Institute of Cosmology and Gravitation, Dennis Sciama Building, University of Portsmouth, Portsmouth, PO1 3FX (United Kingdom)
  • 9. Department of Astronomy and Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, OH 43210 (United States)
  • 10. APC, Université Paris Diderot-Paris 7, CNRS/IN2P3, CEA, Observatoire de Paris, 10, rueA. Domon and L. Duquet, Paris (France)
  • 11. Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349 (United States)

Description

We present the BOSS Lyman-α (Lyα) Forest Sample from SDSS Data Release 9, comprising 54,468 quasar spectra with zqso > 2.15 suitable for Lyα forest analysis. This data set probes the intergalactic medium with absorption redshifts 2.0 < zα < 5.7 over an area of 3275 deg2, and encompasses an approximate comoving volume of 20 h –3 Gpc3. With each spectrum, we have included several products designed to aid in Lyα 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 Lyα 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 Lyα (λ > 1216 Å), extrapolated into the forest region and normalized by a linear function to fit the expected evolution of the Lyα forest mean flux. The estimated continuum errors are ∼< 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 Lyα 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 Lyα forest. The full data set is available from the SDSS-III DR9 Web site.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-6256/145/3/69

Additional details

Identifiers

Publishing Information

Journal Title
Astronomical Journal (New York, N.Y. Online)
Journal Volume
145
Journal Issue
3
Journal Page Range
[16 p.]
ISSN
1538-3881

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
44086017
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ABSORPTION; APPROXIMATIONS; BARYONS; CALIBRATION; CORRECTIONS; DATA ANALYSIS; EMISSION; ERRORS; OSCILLATIONS; QUASARS; RESPIRATORS; SKY; SPECTRA; SPECTROPHOTOMETRY; TRANSMISSION
Descriptors DEC
CALCULATION METHODS; COSMIC RADIO SOURCES; ELEMENTARY PARTICLES; FERMIONS; HADRONS; SORPTION