A DIRECT MEASUREMENT OF THE INTERGALACTIC MEDIUM OPACITY TO H i IONIZING PHOTONS
暂无分享,去创建一个
J. Prochaska | UCOLick Observatory | J. O’Meara | G. Worseck | J. M. O. Imps | Ucsc St. Michael's College | U. Observatory | J. M. O. Imps | Ucsc St. Michael's College
[1] K. Abazajian,et al. THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY , 2008, 0812.0649.
[2] J. Prochaska,et al. ON THE (NON)EVOLUTION OF H i GAS IN GALAXIES OVER COSMIC TIME , 2008, 0811.2003.
[3] L. Trouille,et al. MEASURING THE SOURCES OF THE INTERGALACTIC IONIZING FLUX , 2008, 0811.1042.
[4] Lutz Wisotzki,et al. An unbiased measurement of the UV background and its evolution via the proximity effect in quasar spectra , 2008, 0807.5089.
[5] M. Zaldarriaga,et al. Evolution of the Intergalactic Opacity: Implications for the Ionizing Background, Cosmic Star Formation, and Quasar Activity , 2008, 0807.4177.
[6] J. Prochaska,et al. A Direct Precision Measurement of the Intergalactic Lyα Opacity at 2 ≤ z ≤ 4.2 , 2007, 0710.4522.
[7] A. Mazure,et al. The VVDS type-1 AGN sample: the faint end of the luminosity function , 2007, 0704.1660.
[8] J. Prochaska,et al. The Keck+Magellan Survey for Lyman Limit Absorption. I. The Frequency Distribution of Super Lyman Limit Systems , 2006, astro-ph/0610726.
[9] G. Richards,et al. An Observational Determination of the Bolometric Quasar Luminosity Function , 2006, astro-ph/0605678.
[10] M. White,et al. The effects of ultraviolet background correlations on Lyα forest flux statistics , 2003, astro-ph/0307289.
[11] J. Bullock,et al. Faint Active Galactic Nuclei and the Ionizing Background , 2003 .
[12] J. Miralda-Escudé. On the Evolution of the Ionizing Emissivity of Galaxies and Quasars Required by the Hydrogen Reionization , 2002, astro-ph/0211071.
[13] A. Aguirre,et al. Metallicity of the Intergalactic Medium Using Pixel Statistics. IV. Oxygen , 2002, 0712.1239.
[14] R. Nichol,et al. A Feature at z ∼ 3.2 in the Evolution of the Lyα Forest Optical Depth , 2002, astro-ph/0206293.
[15] M. SubbaRao,et al. Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Quasar Sample , 2002, astro-ph/0202251.
[16] A. F. Davidsen,et al. The Rest-Frame Extreme-Ultraviolet Spectral Properties of Quasi-stellar Objects , 2001, astro-ph/0109531.
[17] Pasadena,et al. The evolution of ΩHI and the epoch of formation of damped Lyman α absorbers , 2001, astro-ph/0107045.
[18] Martin J. Rees,et al. Radiative Transfer in a Clumpy Universe. III. The Nature of Cosmological Ionizing Sources , 1998, astro-ph/9809058.
[19] P. Madau,et al. Radiative Transfer in a Clumpy Universe. II. The Ultraviolet Extragalactic Background , 1995, astro-ph/9509093.
[20] M. Irwin,et al. Evolution of Lyman-limit absorption systems over the redshift range 0.40 < Z < 4.69 , 1994 .
[21] P. Madau,et al. On the photoionization of the intergalactic medium by quasars at high redshift , 1993 .
[22] P. Petitjean,et al. Evidence for structure in the H I column density distribution of QSO absorbers , 1993 .
[23] Kenneth M. Lanzetta,et al. The Evolution of High-redshift Lyman-limit Absorption Systems , 1991 .
[24] Bruce A. Peterson,et al. On the Density of Neutral Hydrogen in Intergalactic Space , 1965 .