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Astronomical library to access planetary ephemeris files

The Stellar Parameters INferred Systematically (SPInS) characterises stars based on classic constraints. It has be derived from the AIMS code. For more details, see https://dreese.pages.obspm.fr/spins

This project contains the deveopment of the compose code only.

Exercises for the parallel computing lectures

Interface Fortran pour simplifier l'utilisation de HDF5

Titan, a code for optically thick and hot photoionised media

Implementation in FORTRAN of the NASA Breakup Model from the paper of Johnson et al. (2001) NASA's new breakup model of EVOLVE 4.0.

Parallel friend of friend halo finder

Spectrum parameters retriever. Uses a line-by-line radiative transfer model coupled with an inversion method.

Convert ephemeris file (.dat) to ascii file compatible with asc2eph

Fortran parallel matrix inversion algorithm. OpenMPI required.