diff --git a/README.md b/README.md index a3b684e..29d6171 100644 --- a/README.md +++ b/README.md @@ -1,10 +1,5 @@ # MIEX for Python -[![arXiv](https://img.shields.io/badge/arXiv-astro--ph%2F0406118-b31b1b)](https://arxiv.org/abs/astro-ph/0406118) -[![ascl](https://img.shields.io/badge/ascl-1810.019-262255)](https://ascl.net/1810.019) -[![bibcode](https://img.shields.io/badge/bibcode-2004CoPhC.162..113W-1c459b)](https://ui.adsabs.harvard.edu/abs/2004CoPhC.162..113W) -[![doi](https://img.shields.io/badge/doi-10.1016%2Fj.cpc.2004.06.070-fab70c)](https://doi.org/10.1016/j.cpc.2004.06.070) - is a Mie scattering code for large grains written in Python and based on [MIEX](https://ui.adsabs.harvard.edu/abs/2018ascl.soft10019W) by [Wolf & Voshchinnikov (2004)](https://ui.adsabs.harvard.edu/abs/2004CoPhC.162..113W). The following quantities for @@ -23,6 +18,14 @@ can be calculated: - Albedo, - Scattering asymmetry factor ($g$). +Modified and ported to Python with permission of S. Wolf. +For the original source code of MIEX written in `FORTRAN90`, we refer to + +[![arXiv](https://img.shields.io/badge/arXiv-astro--ph%2F0406118-b31b1b)](https://arxiv.org/abs/astro-ph/0406118) +[![ascl](https://img.shields.io/badge/ascl-1810.019-262255)](https://ascl.net/1810.019) +[![bibcode](https://img.shields.io/badge/bibcode-2004CoPhC.162..113W-1c459b)](https://ui.adsabs.harvard.edu/abs/2004CoPhC.162..113W) +[![doi](https://img.shields.io/badge/doi-10.1016%2Fj.cpc.2004.06.070-fab70c)](https://doi.org/10.1016/j.cpc.2004.06.070) + ## Requirements @@ -172,5 +175,5 @@ python3 test_miex.py ## Copyright -The original source code written in `FORTRAN90` is distributed under the [CPC license](https://www.elsevier.com/about/policies/open-access-licenses/elsevier-user-license/cpc-license). +The original source code of MIEX written in `FORTRAN90` is distributed under the [CPC license](https://www.elsevier.com/about/policies/open-access-licenses/elsevier-user-license/cpc-license). Modified and ported to Python with permission of S. Wolf.