JADE/CITATION.cff at main · JADE-Exoplanets/JADE · GitHub

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cff-version: 1.2.0
message: "If you use this software, please cite it as below."
authors:
  - family-names: "Attia"
    given-names: "M."
    orcid: "https://orcid.org/0000-0002-7971-7439"
  - family-names: "Bourrier"
    given-names: "V."
    orcid: "https://orcid.org/0000-0002-9148-034X"
  - family-names: "et al."
title: "JADE: Joining Atmosphere and Dynamics for Exoplanets"
version: 1.0.0
date-released: 2021-03-01
doi: 10.5281/zenodo.15167399
url: "https://doi.org/10.5281/zenodo.15167399"
repository-code: "https://github.com/JADE-Exoplanets/JADE"
license: BSD-3-Clause
references:
  - type: article
    authors:
      - family-names: "Attia"
        given-names: "M."
      - family-names: "Bourrier"
        given-names: "V."
      - family-names: "Eggenberger"
        given-names: "P."
      - family-names: "et al."
    title: "The JADE code: Coupling secular exoplanetary dynamics and photo-evaporation"
    journal: "Astronomy & Astrophysics"
    volume: 647
    article-number: A40
    year: 2021
    doi: 10.1051/0004-6361/202039452
    url: "https://doi.org/10.1051/0004-6361/202039452"
preferred-citation:
  type: article
  authors:
    - family-names: "Attia"
      given-names: "M."
    - family-names: "Bourrier"
      given-names: "V."
    - family-names: "Eggenberger"
      given-names: "P."
    - family-names: "et al."
  title: "The JADE code: Coupling secular exoplanetary dynamics and photo-evaporation"
  journal: "Astronomy & Astrophysics"
  volume: 647
  article-number: A40
  year: 2021
  doi: 10.1051/0004-6361/202039452
  url: "https://doi.org/10.1051/0004-6361/202039452"
abstract: >
  JADE (Joining Atmosphere and Dynamics for Exoplanets) couples the most relevant mechanisms affecting close-orbiting exoplanets.
  It simulates the evolution of a hierarchical three-body system to monitor von Zeipel–Lidov–Kozai resonances
  using a secular formalism truncated up to the 4th (hexadecapolar) order. JADE integrates short-range forces dampening the resonance
  (tidal and rotational dissipation, general relativistic precession) while modeling the inner planet as an extended object
  with a complex structure (iron nucleus surrounded by a silicate mantle, topped by an atmosphere of H/He and trace metals).
  The atmosphere dynamically evolves in response to orbital changes, stellar radiation, internal heating, and XUV-induced photo-evaporation.
keywords:
  - exoplanets
  - planetary dynamics
  - hierarchical systems
  - von Zeipel-Lidov-Kozai
  - planetary internal structure
  - atmospheric evolution
  - atmospheric evaporation