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hpparvi authored Nov 14, 2023
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# 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.

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rme.save('map_name.fits')

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© 2023 Hannu Parviainen
© 2023 Hannu Parviainen

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