###############################################################################
# This file is part of SWIFT.
# Copyright (c) 2018 Matthieu Schaller (schaller@strw.leidenuniv.nl)
#
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU Lesser General Public License as published
# by the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
#
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the
# GNU General Public License for more details.
#
# You should have received a copy of the GNU Lesser General Public License
# along with this program.  If not, see <http://www.gnu.org/licenses/>.
#
##############################################################################

# Script used to plot time evolution of gas particle properties. Intended to
# compare result of feedback due to one star placed in centre of uniform box
# of gas with output from EAGLE feedback test. Can also use as input output
# from SWIFT feedback test (tests/testFeedback) with the appropriate change
# to filepath.

import matplotlib

matplotlib.use("Agg")
from pylab import *
from scipy import stats
import h5py
import numpy as np
import glob
import os.path

style.use("../../../tools/stylesheets/mnras.mplstyle")

# Number of snapshots and elements
newest_snap_name = max(glob.glob("stellar_evolution_*.hdf5"))  # , key=os.path.getctime)
n_snapshots = (
    int(newest_snap_name.replace("stellar_evolution_", "").replace(".hdf5", "")) + 1
)
n_elements = 11
n_elements_eagle = 9

# Read the simulation data
sim = h5py.File("stellar_evolution_0000.hdf5", "r")
boxSize = sim["/Header"].attrs["BoxSize"][0]
time = sim["/Header"].attrs["Time"][0]
scheme = sim["/HydroScheme"].attrs["Scheme"]
kernel = sim["/HydroScheme"].attrs["Kernel function"]
neighbours = sim["/HydroScheme"].attrs["Kernel target N_ngb"]
eta = sim["/HydroScheme"].attrs["Kernel eta"]
git = sim["Code"].attrs["Git Revision"]
stellar_mass = sim["/PartType4/Masses"][0]
try:
    E_SNII_cgs = double(sim["/Parameters"].attrs["EAGLEFeedback:SNII_energy_erg"])
    E_SNIa_cgs = double(sim["/Parameters"].attrs["EAGLEFeedback:SNIa_energy_erg"])
    ejecta_vel_cgs = (
        double(sim["/Parameters"].attrs["EAGLEFeedback:AGB_ejecta_velocity_km_p_s"])
        * 1e5
    )
except:
    E_SNII_cgs = double(sim["/Parameters"].attrs["COLIBREFeedback:SNII_energy_erg"])
    E_SNIa_cgs = double(sim["/Parameters"].attrs["COLIBREFeedback:SNIa_energy_erg"])
    ejecta_vel_cgs = (
        double(sim["/Parameters"].attrs["COLIBREFeedback:AGB_ejecta_velocity_km_p_s"])
        * 1e5
    )

try:
    Eu_N_NSM_p_Msun = double(
        sim["/Parameters"].attrs["COLIBREFeedback:num_of_NSM_per_Msun"]
    )
    Eu_N_CEJSN_p_Msun = double(
        sim["/Parameters"].attrs["COLIBREFeedback:num_of_CEJSN_per_Msun"]
    )
    Eu_N_collapsar_p_Msun = double(
        sim["/Parameters"].attrs["COLIBREFeedback:num_of_collapsar_per_Msun"]
    )
    Eu_yield_NSM_Msun = double(
        sim["/Parameters"].attrs["COLIBREFeedback:yield_Eu_from_NSM_event_Msun"]
    )
    Eu_yield_CEJSN_Msun = double(
        sim["/Parameters"].attrs["COLIBREFeedback:yield_Eu_from_CEJSN_event_Msun"]
    )
    Eu_yield_collapsar_Msun = double(
        sim["/Parameters"].attrs["COLIBREFeedback:yield_Eu_from_collapsar_event_Msun"]
    )
except:
    Eu_N_NSM_p_Msun = 0.0
    Eu_N_CEJSN_p_Msun = 0.0
    Eu_N_collapsar_p_Msun = 0.0
    Eu_yield_NSM_Msun = 0.0
    Eu_yield_CEJSN_Msun = 0.0
    Eu_yield_collapsar_Msun = 0.0

# Units
unit_length_in_cgs = sim["/Units"].attrs["Unit length in cgs (U_L)"]
unit_mass_in_cgs = sim["/Units"].attrs["Unit mass in cgs (U_M)"]
unit_time_in_cgs = sim["/Units"].attrs["Unit time in cgs (U_t)"]
unit_temp_in_cgs = sim["/Units"].attrs["Unit temperature in cgs (U_T)"]
unit_vel_in_cgs = unit_length_in_cgs / unit_time_in_cgs
unit_energy_in_cgs = unit_mass_in_cgs * unit_vel_in_cgs * unit_vel_in_cgs
unit_density_in_cgs = unit_mass_in_cgs * unit_length_in_cgs ** -3
unit_pressure_in_cgs = unit_mass_in_cgs / unit_length_in_cgs * unit_time_in_cgs ** -2
unit_int_energy_in_cgs = unit_energy_in_cgs / unit_mass_in_cgs
unit_entropy_in_cgs = unit_energy_in_cgs / unit_temp_in_cgs
yr_in_cgs = sim["PhysicalConstants/CGS"].attrs["year"]
Gyr_in_cgs = sim["PhysicalConstants/CGS"].attrs["year"] * 1e9
Msun_in_cgs = sim["PhysicalConstants/CGS"].attrs["solar_mass"]

# Declare arrays to store SWIFT data
swift_box_gas_mass = zeros(n_snapshots)
swift_box_gas_mass_AGB = zeros(n_snapshots)
swift_box_gas_mass_SNII = zeros(n_snapshots)
swift_box_gas_mass_SNIa = zeros(n_snapshots)
swift_box_star_mass = zeros(n_snapshots)
swift_box_gas_metal_mass = zeros(n_snapshots)
swift_box_gas_metal_mass_AGB = zeros(n_snapshots)
swift_box_gas_metal_mass_SNII = zeros(n_snapshots)
swift_box_gas_metal_mass_SNIa = zeros(n_snapshots)
swift_element_mass = zeros((n_snapshots, n_elements))
swift_rprocess_mass = zeros(n_snapshots)
swift_box_gas_Eu_mass_NSM = zeros(n_snapshots)
swift_box_gas_Eu_mass_CEJSN = zeros(n_snapshots)
swift_box_gas_Eu_mass_Collapsar = zeros(n_snapshots)
swift_internal_energy = zeros(n_snapshots)
swift_kinetic_energy = zeros(n_snapshots)
swift_total_energy = zeros(n_snapshots)
swift_box_mean_Z_z = zeros(n_snapshots)
swift_box_mean_Fe_z = zeros(n_snapshots)
swift_mean_u_start = 0.0
swift_SNIa_rates = zeros(n_snapshots)
t = zeros(n_snapshots)

# Read data from snapshots
for i in range(n_snapshots):
    # print("reading snapshot "+str(i))
    sim = h5py.File("stellar_evolution_%04d.hdf5" % i, "r")
    t[i] = sim["/Header"].attrs["Time"][0]

    masses = sim["/PartType0/Masses"][:]
    swift_box_gas_mass[i] = np.sum(masses)

    try:
        AGB_mass = sim["/PartType0/MassesFromAGB"][:]
        SNII_mass = sim["/PartType0/MassesFromSNII"][:]
        SNIa_mass = sim["/PartType0/MassesFromSNIa"][:]
    except:
        AGB_mass = sim["/PartType0/MassFractionsFromAGB"][:] * masses
        SNII_mass = sim["/PartType0/MassFractionsFromSNII"][:] * masses
        SNIa_mass = sim["/PartType0/MassFractionsFromSNIa"][:] * masses

    swift_box_gas_mass_AGB[i] = np.sum(AGB_mass)
    swift_box_gas_mass_SNII[i] = np.sum(SNII_mass)
    swift_box_gas_mass_SNIa[i] = np.sum(SNIa_mass)

    Z_star = sim["/PartType4/MetalMassFractions"][0]
    star_masses = sim["/PartType4/Masses"][:]
    swift_box_star_mass[i] = np.sum(star_masses)

    metallicities = sim["/PartType0/MetalMassFractions"][:]
    swift_box_gas_metal_mass[i] = np.sum(metallicities * masses)

    AGB_Z_frac = sim["/PartType0/MetalMassFractionsFromAGB"][:]
    SNII_Z_frac = sim["/PartType0/MetalMassFractionsFromSNII"][:]
    SNIa_Z_frac = sim["/PartType0/MetalMassFractionsFromSNIa"][:]

    swift_box_gas_metal_mass_AGB[i] = np.sum(AGB_Z_frac * masses)
    swift_box_gas_metal_mass_SNII[i] = np.sum(SNII_Z_frac * masses)
    swift_box_gas_metal_mass_SNIa[i] = np.sum(SNIa_Z_frac * masses)

    element_abundances = sim["/PartType0/ElementMassFractions"][:][:]
    for j in range(n_elements):
        swift_element_mass[i, j] = np.sum(element_abundances[:, j] * masses)

    try:
        swift_rprocess_mass[i] = np.sum(element_abundances[:, 11] * masses)
        swift_box_gas_Eu_mass_NSM[i] = np.sum(
            sim["/PartType0/MassFractionsFromNSM"][:] * masses
        )
        swift_box_gas_Eu_mass_CEJSN[i] = np.sum(
            sim["/PartType0/MassFractionsFromCEJSN"][:] * masses
        )
        swift_box_gas_Eu_mass_Collapsar[i] = np.sum(
            sim["/PartType0/MassFractionsFromCollapsar"][:] * masses
        )
    except:
        swift_rprocess_mass[i] = 0.0
        swift_box_gas_Eu_mass_NSM[i] = 0.0
        swift_box_gas_Eu_mass_CEJSN[i] = 0.0
        swift_box_gas_Eu_mass_Collapsar[i] = 0.0

    v = sim["/PartType0/Velocities"][:, :]
    v2 = v[:, 0] ** 2 + v[:, 1] ** 2 + v[:, 2] ** 2
    u = sim["/PartType0/InternalEnergies"][:]
    swift_internal_energy[i] = np.sum(masses * u)
    swift_kinetic_energy[i] = np.sum(0.5 * masses * v2)
    swift_total_energy[i] = swift_kinetic_energy[i] + swift_internal_energy[i]

    WeightedTime = sim["/PartType0/MeanMetalWeightedTimes"][:]
    WeightedTime[WeightedTime < 0] = 0
    swift_box_mean_Z_z[i] = np.sum(
        WeightedTime * (metallicities - metallicities[0])
    ) / np.sum(metallicities - metallicities[0])
    swift_box_mean_Z_z[i] *= unit_time_in_cgs / Gyr_in_cgs

    IronFraction = element_abundances[:, 8] - element_abundances[0, 8]
    WeightedTime = sim["/PartType0/MeanIronWeightedTimes"][:]
    WeightedTime[WeightedTime < 0] = 0
    swift_box_mean_Fe_z[i] = np.sum(WeightedTime * IronFraction) / np.sum(IronFraction)
    swift_box_mean_Fe_z[i] *= unit_time_in_cgs / Gyr_in_cgs

    if i == 0:
        swift_mean_u_start = np.mean(u)

    SNIa_rate = sim["/PartType4/SNIaRates"][:]
    swift_SNIa_rates[i] = (
        SNIa_rate
        / (unit_time_in_cgs / Gyr_in_cgs)
        / (swift_box_star_mass[0] * unit_mass_in_cgs / Msun_in_cgs)
    )

    sim.close()


# Read expected yields from EAGLE. Choose which file to use based on metallicity used when
# running SWIFT (can be specified in yml file)
filename = "./StellarEvolutionSolution/Z_%.4f/StellarEvolutionTotal.txt" % Z_star

# Read EAGLE test output
data = loadtxt(filename)
eagle_time_Gyr = data[:, 0]
eagle_total_mass = data[:, 1] * stellar_mass / Msun_in_cgs * unit_mass_in_cgs
eagle_total_metal_mass = data[:, 2] * stellar_mass / Msun_in_cgs * unit_mass_in_cgs
eagle_total_element_mass = (
    data[:, 3 : 3 + n_elements_eagle] * stellar_mass / Msun_in_cgs * unit_mass_in_cgs
)

eagle_energy_from_mass_cgs = (
    eagle_total_mass * Msun_in_cgs * swift_mean_u_start * unit_int_energy_in_cgs
)
eagle_energy_ejecta_cgs = 0.5 * (eagle_total_mass * Msun_in_cgs) * ejecta_vel_cgs ** 2

# Read the mass per channel
filename = "./StellarEvolutionSolution/Z_%.4f/StellarEvolutionAGB.txt" % Z_star
data = loadtxt(filename)
eagle_total_mass_AGB = data[:, 1] * stellar_mass / Msun_in_cgs * unit_mass_in_cgs
eagle_total_metal_mass_AGB = data[:, 2] * stellar_mass / Msun_in_cgs * unit_mass_in_cgs

filename = "./StellarEvolutionSolution/Z_%.4f/StellarEvolutionII.txt" % Z_star
data = loadtxt(filename)
eagle_total_mass_SNII = data[:, 1] * stellar_mass / Msun_in_cgs * unit_mass_in_cgs
eagle_total_metal_mass_SNII = data[:, 2] * stellar_mass / Msun_in_cgs * unit_mass_in_cgs

filename = "./StellarEvolutionSolution/Z_%.4f/StellarEvolutionIa.txt" % Z_star
data = loadtxt(filename)
eagle_total_mass_SNIa = data[:, 1] * stellar_mass / Msun_in_cgs * unit_mass_in_cgs
eagle_total_metal_mass_SNIa = data[:, 2] * stellar_mass / Msun_in_cgs * unit_mass_in_cgs


# Construct Europium expectations
Eu_t = np.linspace(t[0], t[-1], 10000) * unit_time_in_cgs / Gyr_in_cgs
Eu_mass_collapsar_Msun = zeros(np.size(Eu_t))
Eu_mass_CEJSN_Msun = zeros(np.size(Eu_t))
Eu_mass_NSM_Msun = zeros(np.size(Eu_t))

# NSM

t0 = 0.03
t1 = 0.1
mask = Eu_t > t0
Eu_mass_NSM_Msun[mask] = (
    Eu_N_NSM_p_Msun
    * (swift_box_star_mass[0] * unit_mass_in_cgs / Msun_in_cgs)
    * Eu_yield_NSM_Msun
    * np.log(Eu_t[mask] / t0)
)

# Collapsars

t0 = 0.003  # Age of 100 Msun stars with Z = 0.01
t1 = 0.028  # Age of 10 Msun stars with Z = 0.01
mask = np.logical_and(Eu_t > t0, Eu_t <= t1)
Eu_mass_collapsar_Msun[mask] = (
    Eu_N_collapsar_p_Msun
    * (swift_box_star_mass[0] * unit_mass_in_cgs / Msun_in_cgs)
    * Eu_yield_collapsar_Msun
    * (Eu_t[mask] - t0)
    / (t1 - t0)
)
mask = Eu_t > t1
Eu_mass_collapsar_Msun[mask] = (
    Eu_N_collapsar_p_Msun
    * (swift_box_star_mass[0] * unit_mass_in_cgs / Msun_in_cgs)
    * Eu_yield_collapsar_Msun
)

# CEJSN

t0 = 0.003  # Age of 100 Msun stars with Z = 0.01
t1 = 0.076  # Age of 8 Msun stars with Z = 0.01
mask = np.logical_and(Eu_t > t0, Eu_t <= t1)
Eu_mass_CEJSN_Msun[mask] = (
    Eu_N_CEJSN_p_Msun
    * (swift_box_star_mass[0] * unit_mass_in_cgs / Msun_in_cgs)
    * Eu_yield_CEJSN_Msun
    * (Eu_t[mask] - t0)
    / (t1 - t0)
)
mask = Eu_t > t1
Eu_mass_CEJSN_Msun[mask] = (
    Eu_N_CEJSN_p_Msun
    * (swift_box_star_mass[0] * unit_mass_in_cgs / Msun_in_cgs)
    * Eu_yield_CEJSN_Msun
)

# Total Eu mass
Eu_mass_total_Msun = Eu_mass_collapsar_Msun + Eu_mass_CEJSN_Msun + Eu_mass_NSM_Msun


##################

m_Z = swift_box_gas_metal_mass - swift_box_gas_metal_mass[0]
m_Z *= unit_mass_in_cgs / Msun_in_cgs
delta_m_Z = m_Z[1:] - m_Z[:-1]

m_Fe = swift_element_mass[:, 8] - swift_element_mass[0, 8]
m_Fe *= unit_mass_in_cgs / Msun_in_cgs
delta_m_Fe = m_Fe[1:] - m_Fe[:-1]

theory_z_Z = np.zeros(np.size(t))
theory_z_Fe = np.zeros(np.size(t))
for i in range(np.size(t) - 1):
    theory_z_Z[i] = (
        np.sum(delta_m_Z[:i] * t[:i] * unit_time_in_cgs / Gyr_in_cgs) / m_Z[i]
    )
    theory_z_Fe[i] = (
        np.sum(delta_m_Fe[:i] * t[:i] * unit_time_in_cgs / Gyr_in_cgs) / m_Fe[i]
    )

###################

# Plot the interesting quantities
figure(figsize=(7, 7 / 1.6))

suptitle("Star metallicity Z = %.4f" % Z_star)

# Box gas mass --------------------------------
subplot(241)
plot(
    t[1:] * unit_time_in_cgs / Gyr_in_cgs,
    (swift_box_gas_mass[1:] - swift_box_gas_mass[0]) * unit_mass_in_cgs / Msun_in_cgs,
    linewidth=0.5,
    color="k",
    label="Total",
)
plot(
    t * unit_time_in_cgs / Gyr_in_cgs,
    swift_box_gas_mass_AGB * unit_mass_in_cgs / Msun_in_cgs,
    linewidth=0.5,
    color="C0",
    label="AGB",
)
plot(
    t * unit_time_in_cgs / Gyr_in_cgs,
    swift_box_gas_mass_SNII * unit_mass_in_cgs / Msun_in_cgs,
    linewidth=0.5,
    color="C1",
    label="SNII",
)
plot(
    t * unit_time_in_cgs / Gyr_in_cgs,
    swift_box_gas_mass_SNIa * unit_mass_in_cgs / Msun_in_cgs,
    linewidth=0.5,
    color="C2",
    label="SNIa",
)
plot(eagle_time_Gyr[1:], eagle_total_mass[:-1], linewidth=0.5, color="k", ls="--")
plot(eagle_time_Gyr[1:], eagle_total_mass_AGB[:-1], linewidth=0.5, color="C0", ls="--")
plot(eagle_time_Gyr[1:], eagle_total_mass_SNII[:-1], linewidth=0.5, color="C1", ls="--")
plot(eagle_time_Gyr[1:], eagle_total_mass_SNIa[:-1], linewidth=0.5, color="C2", ls="--")
legend(loc="lower right", ncol=2, fontsize=8)
xlabel("${\\rm Time~[Gyr]}$", labelpad=0)
ylabel("Change in total gas particle mass ${[\\rm M_\\odot]}$", labelpad=2)
ticklabel_format(style="sci", axis="y", scilimits=(0, 0))

# Box star mass --------------------------------
subplot(242)
plot(
    t * unit_time_in_cgs / Gyr_in_cgs,
    (swift_box_star_mass) * unit_mass_in_cgs / Msun_in_cgs,
    linewidth=0.5,
    color="k",
    label="COLIBRE",
)
plot(
    eagle_time_Gyr[1:],
    swift_box_star_mass[0] * unit_mass_in_cgs / Msun_in_cgs - eagle_total_mass[:-1],
    linewidth=0.5,
    color="k",
    label="EAGLE",
    ls="--",
)
xlabel("${\\rm Time~[Gyr]}$", labelpad=0)
ylabel("Change in total star particle mass ${[\\rm M_\\odot]}$", labelpad=2)
ticklabel_format(style="sci", axis="y", scilimits=(0, 0))
legend()

# Box gas element  mass --------------------------------
colours = ["k", "r", "g", "b", "c", "y", "m", "skyblue", "plum", "C1", "C2"]
element_names = ["H", "He", "C", "N", "O", "Ne", "Mg", "Si", "Fe", "Sr", "Ba"]
subplot(243)
for j in range(n_elements_eagle):
    plot(
        t[1:] * unit_time_in_cgs / Gyr_in_cgs,
        (swift_element_mass[1:, j] - swift_element_mass[0, j])
        * unit_mass_in_cgs
        / Msun_in_cgs,
        linewidth=0.5,
        color=colours[j],
        ms=0.5,
        label=element_names[j],
    )
for j in range(n_elements_eagle):
    plot(
        eagle_time_Gyr[1:],
        eagle_total_element_mass[:-1, j],
        linewidth=1,
        color=colours[j],
        linestyle="--",
    )
xlabel("${\\rm Time~[Gyr]}$", labelpad=0)
ylabel("Change in element mass of gas particles ${[\\rm M_\\odot]}$", labelpad=2)
xscale("log")
yscale("log")
ylim(
    1e-5 * swift_box_star_mass[0] * unit_mass_in_cgs / Msun_in_cgs,
    swift_box_star_mass[0] * unit_mass_in_cgs / Msun_in_cgs,
)
legend(loc="lower right", ncol=4, fontsize=8, handlelength=1)

subplot(244)
for j in range(n_elements_eagle, n_elements):
    plot(
        t[1:] * unit_time_in_cgs / Gyr_in_cgs,
        (swift_element_mass[1:, j] - swift_element_mass[0, j])
        * unit_mass_in_cgs
        / Msun_in_cgs,
        linewidth=0.5,
        color=colours[j],
        ms=0.5,
        label=element_names[j],
    )
xlabel("${\\rm Time~[Gyr]}$", labelpad=0)
ylabel("Change in element mass of gas particles ${[\\rm M_\\odot]}$", labelpad=2)
xscale("log")
yscale("log")
ylim(
    3e-13 * swift_box_star_mass[0] * unit_mass_in_cgs / Msun_in_cgs,
    3e-7 * swift_box_star_mass[0] * unit_mass_in_cgs / Msun_in_cgs,
)
legend(loc="lower right", ncol=4, fontsize=8, handlelength=1)


subplot(245)  # , xscale="log")
plot(
    t * unit_time_in_cgs / Gyr_in_cgs,
    swift_rprocess_mass * unit_mass_in_cgs / Msun_in_cgs,
    linewidth=0.5,
    color="k",
    label="Total",
)
plot(
    t * unit_time_in_cgs / Gyr_in_cgs,
    swift_box_gas_Eu_mass_NSM * unit_mass_in_cgs / Msun_in_cgs,
    linewidth=0.5,
    color="C2",
    label="NSM",
)
plot(
    t * unit_time_in_cgs / Gyr_in_cgs,
    swift_box_gas_Eu_mass_CEJSN * unit_mass_in_cgs / Msun_in_cgs,
    linewidth=0.5,
    color="C1",
    label="CEJSN",
)
plot(
    t * unit_time_in_cgs / Gyr_in_cgs,
    swift_box_gas_Eu_mass_Collapsar * unit_mass_in_cgs / Msun_in_cgs,
    linewidth=0.5,
    color="C0",
    label="Collapsars",
)
plot(Eu_t, Eu_mass_total_Msun, linewidth=0.5, color="k", ls="--")
plot(Eu_t, Eu_mass_collapsar_Msun, linewidth=0.5, color="C0", ls="--")
plot(Eu_t, Eu_mass_CEJSN_Msun, linewidth=0.5, color="C1", ls="--")
plot(Eu_t, Eu_mass_NSM_Msun, linewidth=0.5, color="C2", ls="--")
legend(loc="upper left", ncol=2, fontsize=8)
xlabel("${\\rm Time~[Gyr]}$", labelpad=0)
ylabel("Change in Europium mass of gas particles ${[\\rm M_\\odot]}$", labelpad=2)

# Box gas metal mass --------------------------------
subplot(246)
plot(
    t[1:] * unit_time_in_cgs / Gyr_in_cgs,
    (swift_box_gas_metal_mass[1:] - swift_box_gas_metal_mass[0])
    * unit_mass_in_cgs
    / Msun_in_cgs,
    linewidth=0.5,
    color="k",
    label="Total",
)
plot(
    t * unit_time_in_cgs / Gyr_in_cgs,
    swift_box_gas_metal_mass_AGB * unit_mass_in_cgs / Msun_in_cgs,
    linewidth=0.5,
    color="C0",
    label="AGB",
)
plot(
    t * unit_time_in_cgs / Gyr_in_cgs,
    swift_box_gas_metal_mass_SNII * unit_mass_in_cgs / Msun_in_cgs,
    linewidth=0.5,
    color="C1",
    label="SNII",
)
plot(
    t * unit_time_in_cgs / Gyr_in_cgs,
    swift_box_gas_metal_mass_SNIa * unit_mass_in_cgs / Msun_in_cgs,
    linewidth=0.5,
    color="C2",
    label="SNIa",
)
plot(eagle_time_Gyr[1:], eagle_total_metal_mass[:-1], linewidth=0.5, color="k", ls="--")
plot(
    eagle_time_Gyr[1:],
    eagle_total_metal_mass_AGB[:-1],
    linewidth=0.5,
    color="C0",
    ls="--",
)
plot(
    eagle_time_Gyr[1:],
    eagle_total_metal_mass_SNII[:-1],
    linewidth=0.5,
    color="C1",
    ls="--",
)
plot(
    eagle_time_Gyr[1:],
    eagle_total_metal_mass_SNIa[:-1],
    linewidth=0.5,
    color="C2",
    ls="--",
)
legend(loc="center right", ncol=2, fontsize=8)
xlabel("${\\rm Time~[Gyr]}$", labelpad=0)
ylabel("Change in total metal mass of gas particles ${[\\rm M_\\odot]}$", labelpad=2)
ticklabel_format(style="sci", axis="y", scilimits=(0, 0))

# Box mass-weighted redshift --------------------------------
subplot(247)
plot(
    t[3:] * unit_time_in_cgs / Gyr_in_cgs,
    swift_box_mean_Fe_z[3:],
    linewidth=0.5,
    color="C1",
    label="Fe",
)
plot(
    t[3:] * unit_time_in_cgs / Gyr_in_cgs,
    theory_z_Fe[3:],
    linewidth=0.5,
    color="C1",
    ls="--",
)
plot(
    t[3:] * unit_time_in_cgs / Gyr_in_cgs,
    swift_box_mean_Z_z[3:],
    linewidth=0.5,
    color="C0",
    label="Z",
)
plot(
    t[3:] * unit_time_in_cgs / Gyr_in_cgs,
    theory_z_Z[3:],
    linewidth=0.5,
    color="C0",
    ls="--",
)
xlabel("${\\rm Time~[Gyr]}$", labelpad=0)
ylabel("Mean time of enrichment~[Gyr]", labelpad=2)
legend(loc="upper left", ncol=1, fontsize=8)


subplot(248)
plot(t * unit_time_in_cgs / Gyr_in_cgs, swift_SNIa_rates, linewidth=0.5, color="C0")
yscale("log")
xlabel("${\\rm Time~[Gyr]}$", labelpad=0)
ylabel("$N_{SNIa}$ / time / solar~mass~$[{\\rm Gyr^{-1}~M_\\odot^{-1}}]$", labelpad=1)

# tight_layout()
savefig("box_evolution_Z_%.4f.png" % (Z_star), dpi=200)