This Jupyter Notebook creates period-radius diagrams with the population-based boundaries of the Neptunian desert, ridge, and savanna derived in Castro-González et al. (2024).
© Elsa Bersier / ERC project SPICE DUNE
You do not need to install anything. You can simply clone or download the repository and run all cells of the nep_des.ipynb file. The code is very straightforward and intuitive to use, so it does not have detailed documentation. If you find any problem or would like to propose an update do not hesitate to drop me an issue, make a pull request, or contact me at acastro@cab.inta-csic.es.
In the left panel, we contextualize some of the best-known planets located in the middle of the Neptunian desert: TOI-849 b (Armstrong et al. 2020), TOI-1853 b (Naponiello et al. 2023), LTT 9779 b (Jenkins et al. 2020), TOI-3071 b (Hacker et al. 2024), TOI-674 b (Murgas et al. 2021), and K2-45 b (Crossfield et al. 2016).
In the right panel, we contextualize a planet in the Neptunian savanna, HATS-17 b (Brahm et al. 2016), and highlight it with a text box. More planets can be depicted similarly.
In the left-hand plot, we used the NASA Exoplanet Archive catalogue, and in the right-hand plot, we used the Exoplanet.eu catalogue. The planetS catalogue for planets with precise masses and radii can also be used.
The contour map represents the observed density of planets in the selected catalogue, which is subjected to different observational and selection biases, and hence it does not represent the true planet occurrence from which the boundaries were derived. We note, however, that there is a quite good (visual) agreement between the observed distribution and the population-based boundaries so it is reasonable to plot them together for visualization purposes.
If you use our population-based mapping of the exo-Neptunian landscape, please give credit to this work:
@ARTICLE{2024A&A...689A.250C,
author = {{Castro-Gonz{\'a}lez}, A. and {Bourrier}, V. and {Lillo-Box}, J. and {Delisle}, J. -B. and {Armstrong}, D.~J. and {Barrado}, D. and {Correia}, A.~C.~M.},
title = "{Mapping the exo-Neptunian landscape: A ridge between the desert and savanna}",
journal = {\aap},
keywords = {planets and satellites: atmospheres, planets and satellites: dynamical evolution and stability, planets and satellites: formation, planets and satellites: gaseous planets, planets and satellites: physical evolution, Astrophysics - Earth and Planetary Astrophysics},
year = 2024,
month = sep,
volume = {689},
eid = {A250},
pages = {A250},
doi = {10.1051/0004-6361/202450957},
archivePrefix = {arXiv},
eprint = {2409.10517},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2024A&A...689A.250C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
If you make use of nep-des to implement the exo-Neptunian boundaries in your research, please also include the following sentence within the acknowledgements section:
This research made use of \texttt{nep-des} (available in \url{https://github.com/castro-gzlz/nep-des})
Please also give credit to the catalogue(s) used: Nasa Exoplanet Archive (Akeson et al. 2013), Exoplanet.eu (Schneider et al. 2011), and/or PlanetS (Otegi et al. 2020; Parc et al. 2024).