halomod.bias.Tinker05¶
- class halomod.bias.Tinker05(nu: numpy.ndarray, delta_c: float = 1.686, m: Optional[numpy.ndarray] = None, mstar: Optional[float] = None, delta_halo: Optional[float] = 200, n: Optional[float] = 1, sigma_8: Optional[float] = 0.8, cosmo: astropy.cosmology.core.FLRW = FlatLambdaCDM(name="Planck15", H0=67.7 km / (Mpc s), Om0=0.307, Tcmb0=2.725 K, Neff=3.05, m_nu=[0. 0. 0.06] eV, Ob0=0.0486), n_eff: Optional[numpy.ndarray] = None, z: float = 0.0, **model_parameters)[source]¶
Empirical bias from Tinker et al (2005).
See documentation for
Bias
for information on input parameters. This model has no free parameters.Notes
This form is the same as that of
SMT01
, however the parameters were re-fit to simulations in [1]. Here the default parameters are(a,b,c) = (0.707, 0.35, 0.8)
.References
- 1
Tinker J. et al., “On the Mass-to-Light Ratio of Large-Scale Structure”, https://ui.adsabs.harvard.edu/abs/2005ApJ…631…41T, 2005
Methods
__init__
(nu[, delta_c, m, mstar, …])Initialize self.
bias
()Calculate the first-order, linear, deterministic halo bias.
Get a dictionary of all implemented models for this component.
Attributes
The HMF model that pairs with this bias in the peak-background split