POSEIDON: A Multidimensional Atmospheric Retrieval Code for Exoplanet Spectra

Fuente: arXiv
Enregistré dans:
Détails bibliographiques
Auteur principal: MacDonald, Ryan J.
Format: Preprint
Publié: 2024
Sujets:
Accès en ligne:
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
_version_ 1866912084035371008
author MacDonald, Ryan J.
author_facet MacDonald, Ryan J.
contents Spectroscopic observations of exoplanet atmospheres can reveal the chemical composition, temperature, cloud properties, and (potentially) the habitability of these distant worlds. The inference of such properties is generally enabled by Bayesian atmospheric retrieval algorithms. However, until recently, many retrieval codes have not been publicly available. Here, we describe the open source release of the POSEIDON exoplanet radiative transfer and retrieval code. POSEIDON is a Python package for the 1D, 2D, or 3D modelling and analysis of exoplanet spectra, which is frequently used to interpret Hubble and JWST observations of exoplanet atmospheres. We provide extensive tutorials on both forward modelling and retrievals in POSEIDON's online documentation, which we hope will serve as a helpful resource for the exoplanet atmosphere community.
format Preprint
id arxiv_https___arxiv_org_abs_2410_18181
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle POSEIDON: A Multidimensional Atmospheric Retrieval Code for Exoplanet Spectra
MacDonald, Ryan J.
Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
Spectroscopic observations of exoplanet atmospheres can reveal the chemical composition, temperature, cloud properties, and (potentially) the habitability of these distant worlds. The inference of such properties is generally enabled by Bayesian atmospheric retrieval algorithms. However, until recently, many retrieval codes have not been publicly available. Here, we describe the open source release of the POSEIDON exoplanet radiative transfer and retrieval code. POSEIDON is a Python package for the 1D, 2D, or 3D modelling and analysis of exoplanet spectra, which is frequently used to interpret Hubble and JWST observations of exoplanet atmospheres. We provide extensive tutorials on both forward modelling and retrievals in POSEIDON's online documentation, which we hope will serve as a helpful resource for the exoplanet atmosphere community.
title POSEIDON: A Multidimensional Atmospheric Retrieval Code for Exoplanet Spectra
topic Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
url https://arxiv.org/abs/2410.18181