  Stellar spectra contain a large amount of information about the conditions in
stellar atmospheres. However, extracting this information is challenging and
demands comprehensive numerical modelling. Here, we present stellar spectra
synthesized using the recently developed state-of-the-art MPS-ATLAS code on a
fine grid of stellar fundamental parameters. These calculations have been
extensively validated against solar and stellar observations and can be used
for various astrophysical applications. The spectra are available at the Max
Planck Digital Library (MPDL,
https://edmond.mpdl.mpg.de/dataset.xhtml?persistentId=doi:10.17617/3.NJ56TR)
and have been also incorporated into the ExoTiC-LD python package
(https://github.com/Exo-TiC/ExoTiC-LD/) which returns stellar limb darkening
coefficients used for the software package Exoplanet Timeseries
Characterisation (ExoTic).
