Continuous statistics of the Lyα forest at 0
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[1] S. López,et al. The Evolution of Lyman-alpha Absorbers in the Redshift Range 0.5 < z < 1.9 , 2006, astro-ph/0608342.
[2] R. Sheth,et al. The probability distribution function of the Lyman α transmitted flux from a sample of Sloan Digital Sky Survey quasars , 2006, astro-ph/0608167.
[3] N. Suzuki,et al. The H I opacity of the intergalactic medium at redshifts 1.6 < z < 3.2 , 2005, astro-ph/0504391.
[4] Wen-Ching,et al. A concordance model of the Lyman α forest at z= 1.95 , 2004, astro-ph/0412557.
[5] N. Suzuki,et al. Cosmological Parameters σ8, the Baryon Density Ωb, the Vacuum Energy Density ΩΛ, the Hubble Constant and the UV Background Intensity from a Calibrated Measurement of H I Lyα Absorption at z = 1.9 , 2004 .
[6] N. Suzuki,et al. The Kast Ground-based Ultraviolet Spectral Survey of 79 Quasi-stellar Objects at Redshift 2 for Lyα Forest and Metal Absorption , 2004, astro-ph/0405051.
[7] A. Songaila. The Evolution of the Intergalactic Medium Transmission to Redshift 6 , 2004, astro-ph/0402347.
[8] N. Suzuki,et al. Predicting QSO Continua in the Lyα Forest , 2003, astro-ph/0306577.
[9] J. Bechtold,et al. Accepted for publication in the Astrophysical Journal A Uniform Analysis of the Ly-α Forest at z = 0 − 5: V. The extragalactic ionizing background at low redshift , 2001 .
[10] J. Bechtold,et al. A uniform analysis of the Lyα forest at z = 0-5. IV. The clustering and evolution of clouds at z ≤ 1.7 , 2001, astro-ph/0111487.
[11] J. Bechtold,et al. A Uniform Analysis of the Lyα Forest at z = 0-5. II. Measuring the Mean Intensity of the Extragalactic Ionizing Background Using the Proximity Effect , 2000, astro-ph/0004155.
[12] S. Penton,et al. The Local Lyα Forest. II. Distribution of H I Absorbers,Doppler Widths, and Baryon Content , 1999, astro-ph/9911128.
[13] P. Mcdonald,et al. The Observed Probability Distribution Function, Power Spectrum, and Correlation Function of the Transmitted Flux in the Lyα Forest , 1999, astro-ph/9911196.
[14] S. Penton,et al. The Local Lyα Forest. I. Observations with the GHRS/G160M on the Hubble Space Telescope , 1999, astro-ph/9911117.
[15] S. V. Penton,et al. The Metagalactic Ionizing Radiation Field at Low Redshift , 1999, astro-ph/9907123.
[16] S. Penton,et al. The Low-redshift Intergalactic Medium , 1999, Publications of the Astronomical Society of Australia.
[17] R. Davé,et al. The Low-Redshift Lyα Forest in Cold Dark Matter Cosmologies , 1998, astro-ph/9807177.
[18] W. Sargent,et al. The Hubble Space Telescope Quasar Absorption Line Key Project. XIV. The Evolution of Lyα Absorption Lines in the Redshift Interval z = 0-1.5 , 1998, astro-ph/9806123.
[19] W. Sargent,et al. The Hubble Space Telescope Quasar Absorption Line Key Project. XIII. A Census of Absorption-Line Systems at Low Redshift , 1998, astro-ph/9805148.
[20] D. Kirkman,et al. Intrinsic Properties of the ⟨z⟩ = 2.7 Lyα Forest from Keck Spectra of Quasar HS 1946+7658 , 1997, astro-ph/9701209.
[21] G. Starkman,et al. Axiorecombination: A New Mechanism for Stellar Axion Production , 1986 .
[22] L. Hernquist,et al. The Opacity of the Lyα Forest and Implications for Ωb and the Ionizing Background , 1996, astro-ph/9612245.
[23] W. Sargent,et al. The Hubble Space Telescope Quasar Absorption Line Key Project. VII. Absorption Systems at Z abs <= 1.3 , 1995, astro-ph/9506124.
[24] S. M. Fall,et al. The proximity effect and the mean intensity of ionizing radiation at low redshifts , 1993 .
[25] George F. Hartig,et al. The Hubble Space Telescope quasar absorption line key project. I - First observational results, including Lyman-alpha and Lyman-limit systems , 1993 .
[26] H. Bi. Lyman-alpha absorption spectrum of the primordial intergalactic medium , 1993 .
[27] J. Ostriker,et al. Lyman-alpha depression of the continuum from high-redshift quasars - A new technique applied in search of the Gunn-Peterson effect , 1991 .
[28] J. B. Oke,et al. Absolute spectrophotometry of very large redshift quasars , 1982 .