  The MAGIC telescopes are one of the three major IACTs (Imaging Atmospheric
Cherenkov Telescopes) for observation of gamma rays in the TeV regime currently
operative. MAGIC functions since 2003, and has published data from more than 60
sources, mostly blazars. MAGIC already provides astronomical \texttt{.fits}
files with basic final scientific products such as spectral energy
distributions, light curves and skymaps from published results. In future, the
format of the files can be complemented with further relevant information to
the community: a) by including the full multi-wavelength dataset enclosed in a
publication, b) providing data in alternative easy-to-use formats such as ASCII
or ECSV, which are accessible with other commonly used packages such as
\texttt{astropy} or \texttt{gammapy}. Finally, besides high level products,
activities have started to provide photon event lists and instrument response
functions in a format such that scientists within and outside the community are
allowed to perform higher level analysis. A second aim is to provide a full
legacy of MAGIC data. This contribution will illustrate the achievements and
plans of this activity.
