coleman-bulge-density-model 0.3.5

A vectorized implementation of the Coleman et al. (2020) Milky Way bulge density model.

Coleman Bulge Density Model

A JAX-based, differentiable implementation of the Coleman et al. (2020) Milky Way bulge density model.

Features

• JAX Backend & Auto-Diff: Built on jax.numpy, allowing for gradient computations via jax.grad.
• Hybrid Evaluation: Evaluates density using jax.scipy.ndimage.map_coordinates for coordinates within a pre-computed grid. It falls back to an analytical model for extrapolation outside the grid bounds.
• Vectorized & JIT-Compiled: Vectorized and JIT-compiled (@jax.jit) to process large arrays of coordinates on CPU, GPU, or TPU.
• Flexible Coordinates: Accepts inputs in either Sun-centered spherical coordinates (r, lat, lon) or Galactic Cartesian coordinates (x, y, z).

Requirements

• Python >= 3.8
• JAX >= 0.4.0
• NumPy >= 1.20.0
• SciPy >= 1.7.0

Installation

This package can be installed using pip:

pip install coleman-bulge-density-model

Usage

To use the model, import the pre-instantiated bulge_density_model.

The returned densities are in units of stars per pc^3, normalised to match the observed VVV star counts in the Ks band.

Basic Evaluation

import jax.numpy as jnp
from coleman_bulge_density import bulge_density_model

# 1. Using Galactic Cartesian coordinates (x, y, z)
density, in_bounds = bulge_density_model(x=8.0, y=0.0, z=0.0)

# 2. Processing large arrays
x_arr = jnp.linspace(0, 15, 100)
y_arr = jnp.zeros(100)
z_arr = jnp.zeros(100)
densities, bounds = bulge_density_model(x=x_arr, y=y_arr, z=z_arr)

HMC & Gradients

The model is compatible with JAX operations, allowing for gradient calculations for use in physics simulations and HMC samplers.

import jax
import jax.numpy as jnp
from coleman_bulge_density import bulge_density_model

def log_prob(position_vector):
    """Calculates the log-probability for a given (x, y, z) position."""
    density, _ = bulge_density_model(
        x=position_vector[0], 
        y=position_vector[1], 
        z=position_vector[2]
    )
    return jnp.log(density)

# Generate the gradient function
grad_log_prob = jax.grad(log_prob)

# Evaluate the gradient at a given position
position = jnp.array([8.0, 0.0, 0.0])
gradient = grad_log_prob(position)