The thermonuclear reaction rates of charged-particle induced reactions have been evaluated and compiled in a seminal, broad community-based effort in the NACRE compilation.
A subset of these reactions have later been re-evaluated by the Brussels nuclear astrophysics group and published under the name NACRE-II.
Parallel to NACRE, the nuclear reactions important for solar hydrogen burning have been evaluated, in a community-based manner, at dedicated workshops: Solar Fusion Cross Sections and Solar Fusion Cross Sections II.
Within ChETEC-INFRA, the scope of this effort has been expanded to include most stable hydrogen burning reactions. These have been evaluated in a community-based effort at the Solar Fusion Cross Sections III workshop in Berkeley, July 22-26, 2022. The evaluated data, fit results, and thermonuclear reaction rates have been published in Reviews of Modern Physics (Solar Fusion III) and is available on Zenodo at this link.
It is planned to add further, community-based evaluated and fitted thermonuclear reaction rates beyond Solar Fusion III in the future.