Thank you for visiting nature.com. You are using a browser version with limited support for CSS. To obtain
the best experience, we recommend you use a more up to date browser (or turn off compatibility mode in
Internet Explorer). In the meantime, to ensure continued support, we are displaying the site without styles
and JavaScript.
Other laboratory (solid lines) and astrophysical (dashed lines) constraints are shown for reference and extracted from ref. 56: CASPEr-ZULF44,53, ChangE31, K-3He (rescaled from gaNN constraints)30 and neutron-star cooling62.