6dFGS¶
Compute the likelihood of supplied D_v or fsigma8(z=0.067)
File |
likelihood/6dfgs/6dfgs_rsd.py |
Attribution |
6dFGS Team |
URL |
|
Citations |
BAO MNRAS 416, 3017 3032 (2011) |
fsigma8 MMNRAS 423, 3430 3444 (2012) |
Assumptions¶
6dFGS dataset
Setup Parameters¶
Name |
Type |
Default |
Description |
---|---|---|---|
feedback |
bool |
False |
Whether to print feedback |
bao_like |
bool |
True |
Whether to use BAO likelihood |
rsd_like |
bool |
False |
Whether to use RSD likelihood |
bao_mode |
str |
rs_dv |
Set to “dv” to use the measurement of D_v or to “rs_dv” to use the ratio r_s/D_v |
mean |
real |
457.0 or 0.423 |
Dv for mode 0 or fsigma8 for mode 1 |
sigma |
real |
27.0 or 0.055 |
Sigma_Dv for mode 0 or sigma_fsigma8 |
redshift |
real |
0.106 or 0.067 |
Redshift of measurements, depending on mode |
Input values¶
Section |
Name |
Type |
Default |
Description |
---|---|---|---|---|
growth_parameters |
d_z |
real 1d |
Linear growth factor D(z) |
|
f_z |
real 1d |
Linear growth rate f(z) |
||
z |
real 1d |
Redshift of samples |
||
cosmological_parameters |
omega_m |
real |
Baryon + cdm density fraction today |
|
sigma_8 |
real |
Amplitude of linear matter power at 8/h Mpc at z=0 |
||
bias |
real |
Galaxy bias |
||
h0 |
real |
Hubble parameter H0/(100 km/s/Mpc) |
||
distances |
z |
real 1d |
Redshifts of samples |
|
d_m |
real 1d |
Physical angular diameter distance in Mpc |
||
h |
real 1d |
Hubble parameter with in units of Mpc |
Output values¶
Section |
Name |
Type |
Description |
---|---|---|---|
likelihoods |
6dfgs_LIKE |
real |
Likelihood of supplied Dv(z=0.106) or fsigma8(z=0.067) |