#import "helpers.typ": *
#import "importer/main.typ": *

#set heading(outlined: false, numbering: none)

= Appendix


== A - Halo mass function of #smallcaps[Thesan-Dark 1] and #smallcaps[Thesan-Dark 2]

#let notebook = json("../workdir/11_visualization/halo_mass_function_thesan_1_2.ipynb")

#figure(
  image_cell(notebook, cell_id: "halo_mass_functions"),
  caption: [
  ]
) <fig:halo_mass_functions>

// TODO - comment


== B - Generation of the cover image
The cover image of this report has been generated using #beorn. From a simulation run with a grid resolution of $512^3$ cells, a slice of the brightness temperature map has been extracted at $z = 8.07$. The slice shows an emission due to the spin temperature being higher than the CMB temperature. The first ionization bubbles appear as dark patches where the ionized hydrogen does not contribute to the 21 cm signal.