Correlation between the mean matter density and the width of the saturated Lyα absorption

被引:2
作者
Zhan, H [1 ]
机构
[1] Univ Arizona, Dept Phys, Tucson, AZ 85721 USA
关键词
quasars : absorption lines; cosmology : theory; large-scale structure of Universe;
D O I
10.1046/j.1365-8711.2003.06883.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report a scaling of the mean matter density with the width of the saturated Lyalpha absorptions. This property is established using the `pseudo-hydro' technique (Croft et al.). It provides a constraint for the inversion of the Lyalpha forest, which encounters difficulty in the saturated region. With a Gaussian density profile and the scaling relation, a simple inversion of the simulated Lyalpha forests shows that the one-dimensional mass power spectrum is well recovered on scales above 2 h(-1) Mpc, or roughly k less than or similar to 0.03 km(-1) s, at z = 3. The recovery underestimates the power on small scales, but improvement is possible with a more sophisticated algorithm.
引用
收藏
页码:935 / 941
页数:7
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