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The KADoNiS (Karlsruhe Astrophysical Database of Nucleosynthesis in Stars)project is an astrophysical online database for cross sections relevant fornucleosynthesis in the $s$ process and the $\gamma$ process. The $s$-processdatabase (www.kadonis.org) was started in 2005 and is presently facing its 4thupdate (KADoNiS v1.0). The $\gamma$-process database (KADoNiS-p,www.kadonis.org/pprocess) was recently revised and re-launched in March 2013.  Both databases are compilations for experimental cross sections withrelevance to heavy ion nucleosynthesis. For the $s$ process recommendedMaxwellian averaged cross sections for $kT$= 5-100~keV are given for more than360 isotopes between $^{1}$H and $^{210}$Bi. For the $\gamma$-process databaseall available experimental data from $(p,\gamma), (p,n), (p,\alpha),(\alpha,\gamma), (\alpha,n)$, and $(\alpha,p)$ reactions between $^{70}$Ge and$^{209}$Bi in or close to the respective Gamow window were collected and can becompared to theoretical predictions. The aim of both databases is a quick anduser-friendly access to the available data in the astrophysically relevantenergy regions.

The Karlsruhe Astrophysical Database of Nucleosynthesis in Stars Project - Status and Prospects