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hpparvi · Nov 15, 2023 · d8d591a · d8d591a
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 [![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)
+[![codecov](https://codecov.io/gh/hpparvi/spright/graph/badge.svg?token=N61LF1M8TL)](https://codecov.io/gh/hpparvi/spright)
 
 Spright (/spraɪt/; Parviainen, Luque, and Palle, accepted to MNRAS) 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