1 """See `cosmolopy.perturbation.transfer_function_EH`
2
3 Eisenstein & Hu power spectrum transfer function used in
4 `cosmolopy.perturbation.transfer_function_EH`.
5
6 This package contains two modules:
7
8 i. `power` (or `cosmolopy.EH.power`), which is a python wrapper of power.c
9 from Eisenstein & Hu (1999 ApJ 511 5)
10
11 ii. `tf_fit` (or `cosmolopy.EH.tf_fit`), which is a python wrapper of
12 tf_fit.c from Eisenstein & Hu (1998 ApJ 496 605)
13
14 The first module contains no baryonic features in the transfer function, but
15 applies to wider range of CDM variants (e.g. including neutrinos). The second
16 module applies more narrowly but possesses effects including the baryonic
17 acoustic osciallations.
18
19 See also: http://background.uchicago.edu/~whu/transfer/transferpage.html
20
21 power.c is redistributed under the MIT License with the permission of
22 Wayne Hu, and is described in Eisenstein, D. J., & Hu, W. "Power
23 Spectra for Cold Dark Matter and Its Variants," 1999, ApJ, 511, 5
24 [astro-ph/9710252]. Please cite this paper to acknowledge use of power
25 spectrum calculations.
26
27 See LISCENSE for additional information.
28
29 """
30