| HAL : in2p3-00742973, version 1 |
| arXiv : 1210.1213 |
| Code Bibliographique ADS : 2012A&A...547L...1N |
| DOI : 10.1051/0004-6361/201220259 |
| Fiche détaillée | Récupérer au format |
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| Astronomy and Astrophysics 547 (2012) L1 |
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| Column density distribution and cosmological mass density of neutral gas: Sloan Digital Sky Survey-III Data Release 9 |
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| SDSS-III Collaboration(s) |
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| (10/2012) |
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| We present the first results from an ongoing survey for Damped Lyman-alpha systems (DLAs) in the spectra of z>2 quasars observed in the course of the Baryon Oscillation Spectroscopic Survey (BOSS), which is part of the Sloan Digital Sky Survey (SDSS) III. Our full (non-statistical) sample, based on Data Release 9, comprises 12,081 systems with log N(HI)>=20, out of which 6,839 have log N(HI)>=20.3. This is the largest DLA sample ever compiled, superseding that from SDSS-II by a factor of seven. Using a statistical sub-sample and estimating systematics from realistic mock data, we probe the N(HI) distribution at = 2.5. Contrary to what is generally believed, the distribution extends beyond 10^22 cm^-2 with a moderate slope of index\approx-3.5. This result matches surprisingly well the opacity-corrected distribution observed at z = 0. The cosmological mass density of neutral gas in DLAs is found to be Omega_g_DLA~10^-3, evolving only mildly over the past 12 billion years. |
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| 1 : | IAP - Institut d'Astrophysique de Paris |
| 2 : | APC - AstroParticule et Cosmologie |
| 3 : | IRFU - Institut de Recherches sur les lois Fondamentales de l'Univers (ex DAPNIA) |
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| APC - Cosmologie et Gravitation |
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| Thème(s) | : | Physique/Astrophysique/Cosmologie et astrophysique extra-galactique Planète et Univers/Astrophysique/Cosmologie et astrophysique extra-galactique |
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| Astrophysics - Cosmology and Extragalactic Astrophysics |
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| Lien vers le texte intégral : |
| in2p3-00742973, version 1 | |
| http://hal.in2p3.fr/in2p3-00742973 | |
| oai:hal.in2p3.fr:in2p3-00742973 | |
| Contributeur : Eric Aubourg | |
| Soumis le : Mercredi 17 Octobre 2012, 17:29:09 | |
| Dernière modification le : Lundi 12 Novembre 2012, 17:49:11 | |