From aac5e204a4d986edade38ba03e1570f1b00534aa Mon Sep 17 00:00:00 2001 From: Hannu Parviainen Date: Tue, 14 Nov 2023 16:01:11 +0000 Subject: [PATCH] Update README.md --- README.md | 8 ++++++-- 1 file changed, 6 insertions(+), 2 deletions(-) diff --git a/README.md b/README.md index 7457e39..6e528e7 100644 --- a/README.md +++ b/README.md @@ -1,6 +1,10 @@ # Spright -Spright (/spraɪt/; Parviainen, Luque, and Palle, submitted to MNRAS) is a fast Bayesian radius-density-mass relation for +[![MNRAS](https://img.shields.io/badge/MNRAS-10.1093/mnras/stad3504-blue.svg)](https://doi.org/10.1093/mnras/stad3504) +[![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) + +Spright (/spraɪt/; Parviainen, Luque, and Palle, accepted to MNRAS) is a fast Bayesian radius-density-mass relation for small planets that allows one to predict planetary masses, densities, and RV semi-amplitudes from an estimate of the planet's radius, or planetary radii given an estimate of the planet's mass. @@ -68,4 +72,4 @@ the parameter uncertainty. rme.save('map_name.fits') --- -© 2023 Hannu Parviainen \ No newline at end of file +© 2023 Hannu Parviainen