skypy.galaxies.morphology.late_type_lognormal_size(magnitude, alpha, beta, gamma, M0, sigma1, sigma2, size=None)[source] [edit on github]

Lognormal size distribution for late-type galaxies.

This function provides a lognormal distribution for the physical size of late-type galaxies, described by equations 12, 15 and 16 in [1].

magnitudefloat or array_like.

Galaxy magnitude at which evaluate the lognormal distribution.

alpha, beta, gamma, M0: float

Model parameters describing the mean size of galaxies in [kpc]. (Equation 15).

sigma1, sigma2: float

Parameters describing the standard deviation of the lognormal distribution for the physical radius of galaxies. (Equation 16).

sizeint or tuple of ints, optional.

Output shape. If the given shape is, e.g., (m, n, k), then m * n * k samples are drawn. If size is None (default), a single value is returned if mean and sigma are both scalars. Otherwise, np.broadcast(mean, sigma).size samples are drawn.

physical_sizenumpy.ndarray or astropy.Quantity

Physical distance for a given galaxy with a given magnitude, in [kpc]. If size is None and magnitude is a scalar, a single sample is returned. If size is ns, different from None, and magnitude is scalar, shape is (ns,). If magnitude has shape (nm,) and size=None, shape is (nm,).



S. Shen, H.J. Mo, S.D.M. White, M.R. Blanton, G. Kauffmann, W. Voges, J. Brinkmann, I. Csabai, Mon. Not. Roy. Astron. Soc. 343, 978 (2003).