Column density distribution and cosmological mass density of neutral gas: Sloan Digital Sky Survey-III Data Release 9

التفاصيل البيبلوغرافية
العنوان: Column density distribution and cosmological mass density of neutral gas: Sloan Digital Sky Survey-III Data Release 9
المؤلفون: Noterdaeme, P., Petitjean, P., Carithers, W. C., Pâris, I., Font-Ribera, A., Bailey, S., Aubourg, E., Bizyaev, D., Ebelke, G., Finley, H., Ge, J., Malanushenko, E., Malanushenko, V., Miralda-Escudé, J., Myers, A. D., Oravetz, D., Pan, K., Pieri, M. M., Ross, N. P., Schneider, D. P., Simmons, A., York, D. G.
سنة النشر: 2012
المجموعة: Astrophysics
مصطلحات موضوعية: Astrophysics - Cosmology and Nongalactic Astrophysics
الوصف: 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.
Comment: Accepted for publication as Letter to the Editor in A&A
نوع الوثيقة: Working Paper
DOI: 10.1051/0004-6361/201220259
URL الوصول: http://arxiv.org/abs/1210.1213
رقم الأكسشن: edsarx.1210.1213
قاعدة البيانات: arXiv
الوصف
DOI:10.1051/0004-6361/201220259