From a3b2924e07ac16808407ed7a474909bd84730dcb Mon Sep 17 00:00:00 2001 From: Hannu Parviainen Date: Sun, 1 Sep 2024 14:39:17 +0100 Subject: [PATCH] Update README.md --- README.md | 3 +++ 1 file changed, 3 insertions(+) diff --git a/README.md b/README.md index 977b9b6..e059775 100644 --- a/README.md +++ b/README.md @@ -4,7 +4,10 @@ [![arXiv](http://img.shields.io/badge/arXiv-2311.07255-blue.svg?style=flat)](https://arxiv.org/abs/2311.07255) [![DOI](https://zenodo.org/badge/DOI/10.5281/zenodo.10082653.svg)](https://doi.org/10.5281/zenodo.10082653) [![Licence](http://img.shields.io/badge/license-GPLv3-blue.svg?style=flat)](http://www.gnu.org/licenses/gpl-3.0.html) +![Python package](https://github.com/hpparvi/spright/actions/workflows/python-package.yml/badge.svg) +[![PyPI version](https://badge.fury.io/py/spright.svg)](https://badge.fury.io/py/spright) [![codecov](https://codecov.io/gh/hpparvi/spright/graph/badge.svg?token=N61LF1M8TL)](https://codecov.io/gh/hpparvi/spright) +[![astropy](http://img.shields.io/badge/powered%20by-AstroPy-orange.svg?style=flat)](http://www.astropy.org/) Spright (/spraɪt/; [Parviainen, Luque, and Palle, 2023](https://doi.org/10.1093/mnras/stad3504)) is a fast Bayesian radius-density-mass relation for small planets. The package allows one to predict planetary masses, densities, and RV semi-amplitudes given the