/PFANT

Stellar Spectral Synthesis code for Astronomy

Primary LanguageFortranGNU General Public License v3.0GPL-3.0

This directory

PFANT
├── fortran . Fortran source code and binaries
├── data .... Some stellar data, spectral lines etc.
├── docs .... Documentation source (Sphinx) 
└── doc ..... Graphic material made in PowerPoint, GIMP etc.

Welcome!

PFANT is a stellar spectral synthesis software for Astronomy.

Installation instructions: http://trevisanj.github.io/PFANT/install.html

PFANT Manual Home: http://trevisanj.github.io/PFANT

References

Barbuy, B. 1982, PhD Thesis, Université de Paris VII

Cayrel, R., Perrin, M. N., Barbuy, B., & Buser, R. (1991). A grid of synthetic spectra for the determination of effective temperature, gravity and metallicity of F, G, and K stars. I-Description of the method. II-Application to 41 stellar spectra taken in the Basel field of SA 141. Astronomy and Astrophysics, 247, 108-129.

Barbuy, B., Perrin, M.-N., Katz, D. et al. 2003, A&A, 404, 661

Coelho, P., Barbuy, B., Meléndez, J., Schiavon, R. P., & Castilho, B. V. (2005). A library of high resolution synthetic stellar spectra from 300 nm to 1.8 μm with solar and α-enhanced composition. Astronomy & Astrophysics, 443(2), 735-746.

Barbuy, B., Trevisan, J., & de Almeida, A. (2018). Calculation of molecular line intensity in stellar atmospheres. arXiv preprint arXiv:1812.02414.