Compare Single star particle to instantaneous SFZH

A sanity check example for a single star in both parametric and particle objects. These should give indistinguishable results.

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/opt/hostedtoolcache/Python/3.10.14/x64/lib/python3.10/site-packages/unyt/array.py:1824: RuntimeWarning: divide by zero encountered in log10
  out_arr = func(np.asarray(inp), out=out_func, **kwargs)

import matplotlib.pyplot as plt
import numpy as np
from matplotlib.colors import Normalize
from mpl_toolkits.axes_grid1 import make_axes_locatable
from synthesizer.grid import Grid
from synthesizer.parametric import Stars as ParametricStars
from synthesizer.particle import Stars as ParticleStars

# Define the grid
grid_name = "test_grid"
grid_dir = "../../tests/test_grid/"
grid = Grid(grid_name, grid_dir=grid_dir)

# Define the parametric stars
stars = ParametricStars(
    grid.log10age,
    grid.metallicity,
    sf_hist=1e7,
    metal_dist=0.01,
    initial_mass=1,
)

# Plot the SFZH
stars.plot_sfzh()

# Compute the parametric sed
sed = stars.get_spectra_transmitted(grid)

# Create the particle stars object
part_stars = ParticleStars(
    initial_masses=np.array([1.0]),
    ages=np.array([1e7]),
    metallicities=np.array([0.01]),
)

# Calculate the particle SFZH grid (equivalent to grid weights)
part_sfzh = part_stars.get_sfzh(grid, grid_assignment_method="cic")

# Plot the SFZH
part_stars.plot_sfzh(grid, grid_assignment_method="cic")

# Create the figure and axes for the comparison
fig, ax = plt.subplots()
ax.grid(True)

# Plot the grid points
x, y = np.meshgrid(grid.log10age, grid.metallicity)
ax.scatter(
    x.flatten(),
    np.log10(y.flatten()),
    marker=".",
    color="grey",
    alpha=0.3,
)

# Plot the stellar particle properties
ax.scatter(
    part_stars.log10ages,
    part_stars.log10metallicities,
    marker="*",
    zorder=10,
    color="gold",
)

# Plot the particle SFZH
plt_part_sfzh = np.full_like(part_sfzh, np.nan)
plt_part_sfzh[part_sfzh > 0] = part_sfzh[part_sfzh > 0]
pcm2 = ax.pcolormesh(
    grid.log10age,
    np.log10(grid.metallicity),
    plt_part_sfzh.T,
    cmap="plasma",
    norm=Normalize(vmin=np.min(part_sfzh[part_sfzh > 0]), vmax=1.0, clip=True),
    alpha=0.8,
)

# Plot the parametric SFZH
plt_para_sfzh = np.full_like(stars.sfzh, np.nan)
plt_para_sfzh[stars.sfzh > 0] = stars.sfzh[stars.sfzh > 0]
pcm1 = ax.pcolormesh(
    grid.log10age,
    np.log10(grid.metallicity),
    plt_para_sfzh.T,
    cmap="Greys_r",
    alpha=0.8,
    norm=Normalize(
        vmin=np.min(stars.sfzh[stars.sfzh > 0]), vmax=1.0, clip=True
    ),
)


# Create colorbars on the right for each mesh
divider = make_axes_locatable(ax)
cax1 = divider.append_axes("right", size="5%", pad=0.1)
cbar1 = fig.colorbar(pcm1, cax=cax1, label="Parametric SFZH")

# Create colorbars on the top for each mesh
cax2 = divider.append_axes("top", size="5%", pad=0.1)
cbar2 = plt.colorbar(
    pcm2,
    cax=cax2,
    orientation="horizontal",
    label="Particle SFZH",
    ticklocation="top",
)

# Label axes
ax.set_xlabel(r"$\log_{10}(\mathrm{Age}/\mathrm{yr})$")
ax.set_ylabel(r"$\log_{10}(Z)$")

plt.show()

part_sed = part_stars.get_spectra_transmitted(
    grid, grid_assignment_method="cic"
)
plt.figure(2)
plt.plot(np.log10(sed.lam), np.log10(sed.lnu), label="parametric")
plt.plot(
    np.log10(part_sed.lam),
    np.log10(part_sed.lnu),
    label="particle",
    linestyle="--",
)
plt.legend()
plt.xlim([2, 5])
plt.ylim([18, 22])
plt.show()