We present a web-based application designed to simulate rotational light curves of small airless Solar System bodies under user-defined geometrical and physical conditions.
Python
SIMBA: A Python-based Single-point Astrochemical Solver And Analysis Tool
Determining molecular abundances in astrophysical environments is crucial for interpreting observational data and constraining physical conditions in these regions. Chemical modelling tools are essential for simulating the complex processes that […]
Signatures Of Planets And Galactic Subpopulations In Solar Analogs. Precise Chemical Abundances With Neural Networks
The aim of this work is to obtain precise atmospheric parameters and chemical abundances automatically for solar twins and analogs to find signatures of exoplanets, as well as to assess […]
archNEMESIS: an Open-source Python Package for Analysis of Planetary Atmospheric Spectra
ArchNEMESIS is an open-source Python package developed for the analysis of remote sensing spectroscopic observations of planetary atmospheres.
easyCHEM: A Python Package For Calculating Chemical Equilibrium Abundances In Exoplanet Atmospheres
For modeling the spectra of exoplanets one must know their atmospheric composition. This is necessary because the abundance of molecules, atoms, ions and condensates is needed to construct the total […]
MultIHeaTS: A Fast and Stable Thermal Solver for Multilayered Planetary Surfaces
A fully implicit scheme is proposed for solving the heat equation in 1D heterogeneous media, available as a computationally efficient open-source Python code. The algorithm uses finite differences on an […]
Gen TSO: A General JWST Simulator for Exoplanet Times-series Observations
Gen TSO is a noise calculator specifically tailored to simulate James Webb Space Telescope (JWST) time-series observations of exoplanets. Gen TSO enables the estimation of signal-to-noise ratios (S/N) for transit […]
NEMESISPY: A Python Package For Simulating And Retrieving Exoplanetary Spectra
NEMESISPY is a Python package developed to perform parametric atmospheric modelling and radiative transfer calculation for the retrievals of exoplanetary spectra.
Revisiting Equilibrium Condensation And Rocky Planet Compositions: Introducing The ECCOplanets Code
We introduce ECCOplanets, an open-source Python code that simulates condensation in the protoplanetary disk.
