phringe 0.1.1

PHRINGE

PHRINGE

PHRINGE is a PHotoelectron counts generatoR for nullING intErferometers capable of generating synthetic data for space-based nulling interferometers. It can simulate the observation of an exoplanetary system and generate realistic data in terms of photoelectron counts as a function of wavelength 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

• Symbolic input of complex amplitude transfer matrix and array positions, ensuring maximum flexibility in architecture modeling
• Symbolic calculation of instrument intensity response
• Noise models for astrophysical noise sources including stellar, local zodi and exozodi leakage
• Noise models for instrumental perturbations including amplitude, phase (OPD) and polarization rotation perturbations
• Export of synthetic 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.