Source code for astrophot.utils.parametric_profiles

import torch
import numpy as np
from .conversions.functions import sersic_n_to_b
from .interpolate import cubic_spline_torch, interp1d_torch


[docs] def sersic_torch(R, n, Re, Ie): """Seric 1d profile function, specifically designed for pytorch operations Parameters: R: Radii tensor at which to evaluate the sersic function n: sersic index restricted to n > 0.36 Re: Effective radius in the same units as R Ie: Effective surface density """ bn = sersic_n_to_b(n) return Ie * torch.exp(-bn * (torch.pow(R / Re, 1 / n) - 1))
[docs] def sersic_np(R, n, Re, Ie): """Sersic 1d profile function, works more generally with numpy operations. In the event that impossible values are passed to the function it returns large values to guide optimizers away from such values. Parameters: R: Radii array at which to evaluate the sersic function n: sersic index restricted to n > 0.36 Re: Effective radius in the same units as R Ie: Effective surface density """ if np.any(np.array([n, Re, Ie]) <= 0): return np.ones(len(R)) * 1e6 bn = sersic_n_to_b(n) return Ie * np.exp(-bn * ((R / Re) ** (1 / n) - 1))
[docs] def gaussian_torch(R, sigma, I0): """Gaussian 1d profile function, specifically designed for pytorch operations. Parameters: R: Radii tensor at which to evaluate the sersic function sigma: standard deviation of the gaussian in the same units as R I0: central surface density """ return (I0 / torch.sqrt(2 * np.pi * sigma ** 2)) * torch.exp( -0.5 * torch.pow(R / sigma, 2) )
[docs] def gaussian_np(R, sigma, I0): """Gaussian 1d profile function, works more generally with numpy operations. Parameters: R: Radii array at which to evaluate the sersic function sigma: standard deviation of the gaussian in the same units as R I0: central surface density """ return (I0 / np.sqrt(2 * np.pi * sigma ** 2)) * np.exp(-0.5 * ((R / sigma) ** 2))
[docs] def exponential_torch(R, Re, Ie): """Exponential 1d profile function, specifically designed for pytorch operations. Parameters: R: Radii tensor at which to evaluate the sersic function Re: Effective radius in the same units as R Ie: Effective surface density """ return Ie * torch.exp( -sersic_n_to_b(torch.tensor(1.0, dtype=R.dtype, device=R.device)) * ((R / Re) - 1.0) )
[docs] def exponential_np(R, Ie, Re): """Exponential 1d profile function, works more generally with numpy operations. Parameters: R: Radii array at which to evaluate the sersic function Re: Effective radius in the same units as R Ie: Effective surface density """ return Ie * np.exp(-sersic_n_to_b(1.0) * (R / Re - 1.0))
[docs] def moffat_torch(R, n, Rd, I0): """Moffat 1d profile function, specifically designed for pytorch operations Parameters: R: Radii tensor at which to evaluate the moffat function n: concentration index Rd: scale length in the same units as R I0: central surface density """ return I0 / (1 + (R / Rd) ** 2) ** n
[docs] def moffat_np(R, n, Rd, I0): """Moffat 1d profile function, works with numpy operations. Parameters: R: Radii tensor at which to evaluate the moffat function n: concentration index Rd: scale length in the same units as R I0: central surface density """ return I0 / (1 + (R / Rd) ** 2) ** n
[docs] def nuker_torch(R, Rb, Ib, alpha, beta, gamma): """Nuker 1d profile function, specifically designed for pytorch operations Parameters: R: Radii tensor at which to evaluate the nuker function Ib: brightness at the scale length, represented as the log of the brightness divided by pixel scale squared. Rb: scale length radius alpha: sharpness of transition between power law slopes beta: outer power law slope gamma: inner power law slope """ return ( Ib * (2 ** ((beta - gamma) / alpha)) * ((R / Rb) ** (-gamma)) * ((1 + (R / Rb) ** alpha) ** ((gamma - beta) / alpha)) )
[docs] def nuker_np(R, Rb, Ib, alpha, beta, gamma): """Nuker 1d profile function, works with numpy functions Parameters: R: Radii tensor at which to evaluate the nuker function Ib: brightness at the scale length, represented as the log of the brightness divided by pixel scale squared. Rb: scale length radius alpha: sharpness of transition between power law slopes beta: outer power law slope gamma: inner power law slope """ return ( Ib * (2 ** ((beta - gamma) / alpha)) * ((R / Rb) ** (-gamma)) * ((1 + (R / Rb) ** alpha) ** ((gamma - beta) / alpha)) )
[docs] def spline_torch(R, profR, profI, extend): """Spline 1d profile function, cubic spline between points up to second last point beyond which is linear, specifically designed for pytorch. Parameters: R: Radii tensor at which to evaluate the sersic function profR: radius values for the surface density profile in the same units as R profI: surface density values for the surface density profile """ I = cubic_spline_torch(profR, profI, R.view(-1), extend="none").view(*R.shape) res = torch.zeros_like(I) res[R <= profR[-1]] = 10 ** (I[R <= profR[-1]]) if extend: res[R > profR[-1]] = 10 ** ( profI[-2] + (R[R > profR[-1]] - profR[-2]) * ((profI[-1] - profI[-2]) / (profR[-1] - profR[-2])) ) else: res[R > profR[-1]] = 0 return res