MAOPPY
Modelization of the Adaptive Optics Psf in PYthon
Library for parsimonious modelization of the PSF for astronomy applications.
It includes the Moffat
model (Moffat 1969) and the Psfao
model (Fétick+2019b, see full reference below) dedicated to a modelization of the AO corrected PSF.
The instruments zimpol
, muse_nfm
and papyrus
are already implemented, but feel free to add yours. Do not hesitate to contact me (information below) if you wish to contribute or add a major instrument to MAOPPY.
Quick start
Read the maoppy_user_manual.pdf to see how to download, install and use MAOPPY
Author
Romain JL. Fétick (romain.fetick@lam.fr)
Laboratoire d'Astrophysique de Marseille / ONERA Salon-de-Provence
38 rue Frédéric Joliot Curie, 13388 Marseille (France)
References
The Psfao
model of this library is fully described in the publication:
More developments on the Psfao
model:
Scientific applications:
- STARFINDER2 Schreiber et al., Dec. 2020, SPIE proceedings, Vol.11448
- photometry Massari et al., Dec. 2020, SPIE proceedings, Vol.11448
- deconvolution Fétick et al., July 2020, MNRAS, Vol.496
- PSF extraction in crowded field Gottgens et al., Aug. 2021, MNRAS, Vol.507
License
See the LICENSE file