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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