phringe 0.0.12

PHRINGE

PHRINGE

PHRINGE is a synthetic PHotometRy data generator for nullING intErferometers. It can simulate the observation of an exoplanetary system with a space-based nulling interferometer and generate realistic photometry data as a function of wavelength/spectral channel and time, considering both astrophysical and instrumental noise sources.

Documentation

The documentation including installation and usage instructions, examples and a general user documentation can be found on phringe.readthedocs.io.

Features

• Model different array architectures including different array configurations (Emma-X, Triangle, Pentagon) and different nulling schemes (double Bracewell, Kernel)
• Model noise contributions from astrophysical sources including stellar, local zodi and exozodi leakage
• Model noise contributions from systematic instrument perturbations including amplitude, phase (OPD) and polarization rotation perturbations
• Configure the osbervation and the observatory with all major parameters
• Configure the observed planetary system including the star, planets and exozodi
• Export the photometry data as a FITS file

Contributing

Contributions are very welcome. To learn more, see the Contributor Guide.

License

Distributed under the terms of the MIT license, PHRINGE is free and open source software.

Issues

If you encounter any problems, please file an issue along with a detailed description.

Credits

This project was generated from @cjolowicz's Hypermodern Python Cookiecutter template.