41 lines
1.9 KiB
Plaintext
41 lines
1.9 KiB
Plaintext
# %ECSV 1.0
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# ---
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# datatype:
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# - {name: name, datatype: string}
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# - {name: H0, unit: km / (Mpc s), datatype: float64, format: '', description: Hubble constant as an `~astropy.units.Quantity` at z=0.}
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# - {name: Om0, datatype: float64, format: '', description: Omega matter; matter density/critical density at z=0.}
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# - {name: Tcmb0, unit: K, datatype: float64, format: '', description: Temperature of the CMB as `~astropy.units.Quantity` at z=0.}
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# - {name: Neff, datatype: float64, format: '', description: Number of effective neutrino species.}
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# - {name: m_nu, unit: eV, datatype: string, format: '', description: Mass of neutrino species., subtype: 'float64[3]'}
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# - {name: Ob0, datatype: float64, format: '', description: Omega baryon; baryonic matter density/critical density at z=0.}
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# meta: !!omap
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# - {Oc0: 0.23}
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# - {n: 0.946}
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# - {sigma8: 0.784}
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# - {tau: 0.079}
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# - z_reion: !astropy.units.Quantity
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# unit: !astropy.units.Unit {unit: redshift}
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# value: 10.3
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# - t0: !astropy.units.Quantity
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# unit: !astropy.units.Unit {unit: Gyr}
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# value: 13.78
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# - {reference: 'Spergel et al. 2007, ApJS, 170, 377, doi: 10.1086/513700. Table 6 (WMAP + SNGold) obtained from: https://lambda.gsfc.nasa.gov/product/map/dr2/params/lcdm_wmap_sngold.cfm \nPending
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# WMAP team approval and subject to change.'}
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# - {cosmology: FlatLambdaCDM}
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# - __serialized_columns__:
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# H0:
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# __class__: astropy.units.quantity.Quantity
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# unit: !astropy.units.Unit {unit: km / (Mpc s)}
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# value: !astropy.table.SerializedColumn {name: H0}
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# Tcmb0:
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# __class__: astropy.units.quantity.Quantity
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# unit: !astropy.units.Unit {unit: K}
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# value: !astropy.table.SerializedColumn {name: Tcmb0}
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# m_nu:
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# __class__: astropy.units.quantity.Quantity
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# unit: !astropy.units.Unit {unit: eV}
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# value: !astropy.table.SerializedColumn {name: m_nu}
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# schema: astropy-2.0
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name H0 Om0 Tcmb0 Neff m_nu Ob0
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WMAP3 70.1 0.276 2.725 3.04 [0.0,0.0,0.0] 0.0454
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