Titan, a code for optically thick and hot photoionised media
Passing on the development environment from the AITC Summer Research Scholarship 2019 (Kraken GUI Project).
Namespace for TFCat
Public Website: https://streams.pages.obspm.fr/streams/
Quantifying how indicative the stellar stream is of the orbit of the host
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
Python package to deal with NAIF SPICE kernels for Solar Orbiter
Program to deal with NAIF SPICE kernels for Solar Orbiter