  The KADoNiS (Karlsruhe Astrophysical Database of Nucleosynthesis in Stars)
project is an astrophysical online database for cross sections relevant for
nucleosynthesis in the $s$ process and the $\gamma$ process. The $s$-process
database (www.kadonis.org) was started in 2005 and is presently facing its 4th
update (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 with
relevance to heavy ion nucleosynthesis. For the $s$ process recommended
Maxwellian averaged cross sections for $kT$= 5-100~keV are given for more than
360 isotopes between $^{1}$H and $^{210}$Bi. For the $\gamma$-process database
all 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 be
compared to theoretical predictions. The aim of both databases is a quick and
user-friendly access to the available data in the astrophysically relevant
energy regions.
