Included Cosmology Realizations#
A number of preloaded cosmologies are available from analyses using the WMAP and
Planck satellite data. The full list of the predefined cosmologies is given by
cosmology.realizations.available
and summarized below:
Name |
Source |
H0 |
Om |
Flat |
---|---|---|---|---|
Spergel et al. 2003 |
72.0 |
0.257 |
Yes |
|
Spergel et al. 2007 |
70.1 |
0.276 |
Yes |
|
Komatsu et al. 2009 |
70.2 |
0.277 |
Yes |
|
Komatsu et al. 2011 |
70.4 |
0.272 |
Yes |
|
Hinshaw et al. 2013 |
69.3 |
0.287 |
Yes |
|
Planck Collab 2013, Paper XVI |
67.8 |
0.307 |
Yes |
|
Planck Collab 2015, Paper XIII |
67.7 |
0.307 |
Yes |
|
Planck Collab 2018, Paper VI |
67.7 |
0.310 |
Yes |
Currently, all are instances of FlatLambdaCDM
. More details about exactly
where each set of parameters comes from are available in the docstring for each
object and described below:
>>> from astropy.cosmology import WMAP7
>>> print(WMAP7.__doc__)
WMAP7 instance of FlatLambdaCDM cosmology
(from Komatsu et al. 2011, ApJS, 192, 18, doi: 10.1088/0067-0049/192/2/18.
Table 1 (WMAP + BAO + H0 ML).)
Planck 2018#
The parameters are from Planck Collaboration (2020) Table 2 (TT, TE, EE + lowE + lensing + BAO) [P18].
Note
The Planck 2018 paper includes massive neutrinos in Om0
but the Planck18
object includes them in m_nu
instead for consistency. Hence, the Om0
value in Planck18 differs slightly from the Planck 2018 paper but represents
the same cosmological model.
Metadata#
Oc0 |
Omega cold dark matter at z=0 |
n |
Density perturbation spectral index |
sigma8 |
Density perturbation amplitude |
tau |
Ionisation optical depth |
z_reion |
Redshift of hydrogen reionisation |
t0 |
Age of the universe in Gyr |
reference |
Reference for the parameters |
References#
Planck Collaboration, et. al. (2020). Planck 2018 results. VI. Cosmological parameters. Astronomy & Astrophysics, 641, A6. https://ui.adsabs.harvard.edu/abs/2020A%26A…641A…6P/abstract
Planck 2015#
Parameters are from Planck Collaboration (2016) Paper XIII, Table 4 (TT, TE, EE + lowP + lensing + ext) [P15].
Metadata#
Oc0 |
Omega cold dark matter at z=0 |
n |
Density perturbation spectral index |
sigma8 |
Density perturbation amplitude |
tau |
Ionisation optical depth |
z_reion |
Redshift of hydrogen reionisation |
t0 |
Age of the universe in Gyr |
reference |
Reference for the parameters |
References#
Planck Collaboration, et. al. (2016). Planck 2015 results. XIII. Cosmological parameters. Astronomy & Astrophysics, 594, A13. https://ui.adsabs.harvard.edu/abs/2016A%26A…594A..13P/abstract
Planck 2013#
Parameters are from Planck Collaboration (2014) Paper XVI, Table 5 (Planck + WP + highL + BAO) [P13].
Metadata#
Oc0 |
Omega cold dark matter at z=0 |
n |
Density perturbation spectral index |
sigma8 |
Density perturbation amplitude |
tau |
Ionisation optical depth |
z_reion |
Redshift of hydrogen reionisation |
t0 |
Age of the universe in Gyr |
reference |
Reference for the parameters |
References#
Planck Collaboration, et. al. (2014). Planck 2013 results. XVI. Cosmological parameters. Astronomy & Astrophysics, 571, A16. https://ui.adsabs.harvard.edu/abs/2014A%26A…571A..16P/abstract
WMAP 9 Year#
Parameters are from Hinshaw et al. (2013) Table 4 (WMAP9 + eCMB + BAO + H0) [WM9].
Metadata#
Oc0 |
Omega cold dark matter at z=0 |
n |
Density perturbation spectral index |
sigma8 |
Density perturbation amplitude |
tau |
Ionisation optical depth |
z_reion |
Redshift of hydrogen reionisation |
t0 |
Age of the universe in Gyr |
reference |
Reference for the parameters |
References#
Hinshaw, G., Larson, D., Komatsu, E., Spergel, D., Bennett, C., Dunkley, J., Nolta, M., Halpern, M., Hill, R., Odegard, N., Page, L., Smith, K., Weiland, J., Gold, B., Jarosik, N., Kogut, A., Limon, M., Meyer, S., Tucker, G., Wollack, E., & Wright, E. (2013). Nine-year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results. The Astrophysical Journal Supplement, 208(2), 19. https://ui.adsabs.harvard.edu/abs/2014A%26A…571A..16P/abstract
WMAP 7 Year#
Parameters are from Komatsu et al. (2011) Table 1 (WMAP + BAO + H0 ML) [WM7].
Metadata#
Oc0 |
Omega cold dark matter at z=0 |
n |
Density perturbation spectral index |
sigma8 |
Density perturbation amplitude |
tau |
Ionisation optical depth |
z_reion |
Redshift of hydrogen reionisation |
t0 |
Age of the universe in Gyr |
reference |
Reference for the parameters |
References#
Komatsu, E., Smith, K., Dunkley, J., Bennett, C., Gold, B., Hinshaw, G., Jarosik, N., Larson, D., Nolta, M., Page, L., Spergel, D., Halpern, M., Hill, R., Kogut, A., Limon, M., Meyer, S., Odegard, N., Tucker, G., Weiland, J., Wollack, E., & Wright, E. (2011). Seven-year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation. The Astrophysical Journal Supplement, 192(2), 18. https://ui.adsabs.harvard.edu/abs/2011ApJS..192…18K/abstract
WMAP 5 Year#
Parameters are from Komatsu et al. (2009) Table 1 (WMAP + BAO + SN ML) [WM5].
Metadata#
Oc0 |
Omega cold dark matter at z=0 |
n |
Density perturbation spectral index |
sigma8 |
Density perturbation amplitude |
tau |
Ionisation optical depth |
z_reion |
Redshift of hydrogen reionisation |
t0 |
Age of the universe in Gyr |
reference |
Reference for the parameters |
References#
Komatsu, E., Dunkley, J., Nolta, M., Bennett, C., Gold, B., Hinshaw, G., Jarosik, N., Larson, D., Limon, M., Page, L., Spergel, D., Halpern, M., Hill, R., Kogut, A., Meyer, S., Tucker, G., Weiland, J., Wollack, E., & Wright, E. (2009). Five-Year Wilkinson Microwave Anisotropy Probe Observations: Cosmological Interpretation. The Astrophysical Journal Supplement, 180(2), 330-376. https://ui.adsabs.harvard.edu/abs/2009ApJS..180..330K/abstract
WMAP 3 Year#
Parameters are from Spergel et al. (2007) Table 6 (WMAP + SNGold) [WM3],
obtained from
https://lambda.gsfc.nasa.gov/product/map/dr2/params/lcdm_wmap_sngold.cfm.
Tcmb0
and Neff
are the standard values as also used for WMAP 5 Year,
WMAP 7 Year, WMAP 9 Year.
Note
Pending WMAP team approval and subject to change.
Metadata#
Oc0 |
Omega cold dark matter at z=0 |
n |
Density perturbation spectral index |
sigma8 |
Density perturbation amplitude |
tau |
Ionisation optical depth |
z_reion |
Redshift of hydrogen reionisation |
t0 |
Age of the universe in Gyr |
reference |
Reference for the parameters |
References#
Spergel, D., Bean, R., Doré, O., Nolta, M., Bennett, C., Dunkley, J., Hinshaw, G., Jarosik, N., Komatsu, E., Page, L., Peiris, H., Verde, L., Halpern, M., Hill, R., Kogut, A., Limon, M., Meyer, S., Odegard, N., Tucker, G., Weiland, J., Wollack, E., & Wright, E. (2007). Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Cosmology. The Astrophysical Journal Supplement, 170(2), 377-408. https://ui.adsabs.harvard.edu/abs/2007ApJS..170..377S/abstract
WMAP 1 Year#
Parameters are from Spergel et al. (2003) Table 7 (WMAP + CBI + ACBAR + 2dFGRS
+ Lya) [WM1]. Tcmb0
and Neff
are the standard values as also used for
WMAP 5 Year, WMAP 7 Year, WMAP 9 Year.
Note
Pending WMAP team approval and subject to change.
Metadata#
Oc0 |
Omega cold dark matter at z=0 |
n |
Density perturbation spectral index |
sigma8 |
Density perturbation amplitude |
tau |
Ionisation optical depth |
z_reion |
Redshift of hydrogen reionisation |
t0 |
Age of the universe in Gyr |
reference |
Reference for the parameters |
References#
Spergel, D., Verde, L., Peiris, H., Komatsu, E., Nolta, M., Bennett, C., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., Limon, M., Meyer, S., Page, L., Tucker, G., Weiland, J., Wollack, E., & Wright, E. (2003). First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters. The Astrophysical Journal Supplement, 148(1), 175-194. https://ui.adsabs.harvard.edu/abs/2003ApJS..148..175S/abstract
Reference/API#
astropy.cosmology.realizations Module#
Classes#
The default cosmology to use. |
Variables#
Built-in immutable sequence. |
|
WMAP1 instance of FlatLambdaCDM cosmology (from Spergel et al. 2003, ApJS, 148, 175, doi: 10.1086/377226. |
|
WMAP3 instance of FlatLambdaCDM cosmology (from Spergel et al. 2007, ApJS, 170, 377, doi: 10.1086/513700. |
|
WMAP5 instance of FlatLambdaCDM cosmology (from Komatsu et al. 2009, ApJS, 180, 330, doi: 10.1088/0067-0049/180/2/330. |
|
WMAP7 instance of FlatLambdaCDM cosmology (from Komatsu et al. 2011, ApJS, 192, 18, doi: 10.1088/0067-0049/192/2/18. |
|
WMAP9 instance of FlatLambdaCDM cosmology (from Hinshaw et al. 2013, ApJS, 208, 19, doi: 10.1088/0067-0049/208/2/19. |
|
Planck13 instance of FlatLambdaCDM cosmology (from Planck Collaboration 2014, A&A, 571, A16 (Paper XVI), Table 5 (Planck + WP + highL + BAO)) |
|
Planck15 instance of FlatLambdaCDM cosmology (from Planck Collaboration 2016, A&A, 594, A13 (Paper XIII), Table 4 (TT, TE, EE + lowP + lensing + ext)) |
|
Planck18 instance of FlatLambdaCDM cosmology (from Planck Collaboration 2018, 2020, A&A, 641, A6 (Paper VI), Table 2 (TT, TE, EE + lowE + lensing + BAO)) |