Introduction | Usage | TauREx 3 | Citing ACEPython
ACEPython is a Python wrapper for the FORTRAN equilibrium chemistry code developed by Agúndez et al. 2012. It can rapidly compute the equilibirum chemical scheme for a given temperature and pressure.
ACEPython can be installed with prebuilt wheels using pip:
pip install acepythonOr, if you prefer, you can build it from source which requires a FORTRAN and C compiler. The following commands will build and install ACEPython:
git clone https://github.com/ucl-exoplanets/acepython.git
cd acepython
pip install .ACEPython can be used to compute the equilibrium chemistry for a given temperature and pressure. Temperature and pressure must be created with astropy units. For pressure, any unit can be used (Pa, bar etc). The following example shows how to compute the equilibrium chemistry for a column of atmosphere:
from acepython import run_ace
from astropy import units as u
import numpy as np
import matplotlib.pyplot as plt
temperature = np.linspace(3000, 1000, 100) << u.K
pressure = np.logspace(6, -2, 100) << u.bar
species, mix_profile, mu_profile = run_ace(
temperature,
pressure,
)
species_to_see = ["H2", "H20", "CH4", "NH3", "C2H2", "CO", "CO2", "H2CO"]
fig, (ax1, ax2) = plt.subplots(1, 2, figsize=(10, 5))
for i, spec in enumerate(species):
if spec in species_to_see:
ax1.plot(mix_profile[i], pressure, label=spec)
ax1.set_yscale("log")
ax1.set_xscale("log")
ax1.invert_yaxis()
ax1.set_ylabel("Pressure (bar)")
ax1.set_xlabel("VMR")
ax1.legend()
ax2.plot(mu_profile, pressure)
ax2.set_yscale("log")
ax2.invert_yaxis()
ax2.set_ylabel("Pressure (bar)")
ax2.set_xlabel("Mean molecular weight (au)")
plt.show()Should produce the following figure:
By default the elements in the chemical scheme are H, He, C, N, O at log abundances 12, 10.93, 8.39, 7.86, 8.73 respectively. The abundances can be changed by passing the elements and corresponding abundances to the run_ace function:
species, mix_profile, mu_profile = run_ace(
temperature,
pressure,
elements=["H", "He", "C", "N", "O"],
abundances=[12, 10.93, 8.39, 7.86, 7.73],
)where we have changed O to have a log abundance of 7.73.
You can customize the species included by passing in thermochemical and species data files.
For example, if we have a custom thermochemical data file called custom_thermochemical_data.dat and a custom species data file called custom_species_data.dat that includes sulphur we can run ACEPython with:
species, mix_profile, mu_profile = run_ace(
temperature,
pressure,
elements=["H", "He", "C", "N", "O", "S"],
abundances=[12, 10.93, 8.39, 7.86, 7.73, 7.0],
thermochemical_data="custom_thermochemical_data_w_S.dat",
species_data="custom_species_data_w_S.dat",
)ACEPython also includes a plugin for TauREx 3.1 that allows you to use ACEPython as a chemistry scheme. In the input file you can select it in the Chemistry section using acepython with arguments:
[Chemistry]
chemistry = acepython
# He/H ratio (optional)
he_h_ratio = 0.83
# Elements excluding H, He (optional)
elements = C, N, O
# log abundances (optional)
abundances = 8.39, 7.86, 8.73
# Custom species data file (optional)
spec_file = custom_species_data.dat
# Custom thermochemical data file (optional)
thermo_file = custom_thermochemical_data.dat If you use ACEPython in your research, please cite the following papers:
@ARTICLE{Agundez2012,
author = {{Ag{\'u}ndez}, M. and {Venot}, O. and {Iro}, N. and {Selsis}, F. and
{Hersant}, F. and {H{'e}brard}, E. and {Dobrijevic}, M.},
title = "{The impact of atmospheric circulation on the chemistry of the hot Jupiter HD 209458b}",
journal = {A\&A},
keywords = {astrochemistry, planets and satellites: atmospheres, planets and satellites: individual: HD 209458b, Astrophysics - Earth and Planetary Astrophysics},
year = "2012",
month = "Dec",
volume = {548},
eid = {A73},
pages = {A73},
doi = {10.1051/0004-6361/201220365},
archivePrefix = {arXiv},
eprint = {1210.6627},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2012A&A...548A..73A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2021ApJ...917...37A,
author = {{Al-Refaie}, A.~F. and {Changeat}, Q. and {Waldmann}, I.~P. and {Tinetti}, G.},
title = "{TauREx 3: A Fast, Dynamic, and Extendable Framework for Retrievals}",
journal = {\apj},
keywords = {Open source software, Astronomy software, Exoplanet atmospheres, Radiative transfer, Bayesian statistics, Planetary atmospheres, Planetary science, 1866, 1855, 487, 1335, 1900, 1244, 1255, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics},
year = 2021,
month = aug,
volume = {917},
number = {1},
eid = {37},
pages = {37},
doi = {10.3847/1538-4357/ac0252},
archivePrefix = {arXiv},
eprint = {1912.07759},
primaryClass = {astro-ph.IM},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJ...917...37A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2022ApJ...932..123A,
author = {{Al-Refaie}, A.~F. and {Changeat}, Q. and {Venot}, O. and {Waldmann}, I.~P. and {Tinetti}, G.},
title = "{A Comparison of Chemical Models of Exoplanet Atmospheres Enabled by TauREx 3.1}",
journal = {\apj},
keywords = {Open source software, Publicly available software, Chemical abundances, Bayesian statistics, Exoplanet atmospheres, Exoplanet astronomy, Exoplanet atmospheric composition, Exoplanets, Radiative transfer, 1866, 1864, 224, 1900, 487, 486, 2021, 498, 1335, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
year = 2022,
month = jun,
volume = {932},
number = {2},
eid = {123},
pages = {123},
doi = {10.3847/1538-4357/ac6dcd},
archivePrefix = {arXiv},
eprint = {2110.01271},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2022ApJ...932..123A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
