Explore projects
-
Astronomical library to access planetary ephemeris files
Updated -
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
Updated -
This project contains the deveopment of the compose code only.
Updated -
-
Interface Fortran pour simplifier l'utilisation de HDF5
Updated -
Titan, a code for optically thick and hot photoionised media
Updated -
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.
Updated -
Parallel friend of friend halo finder
Updated -
Spectrum parameters retriever. Uses a line-by-line radiative transfer model coupled with an inversion method.
Updated -
Convert ephemeris file (.dat) to ascii file compatible with asc2eph
Updated -
Fortran parallel matrix inversion algorithm. OpenMPI required.
Updated