We present the first results of application of the MANCHA3D code (Felipe 2010; Khomenko et al. 2017, 2018) to a K0V cool star. Initially we run the code solving purely hydrodynamic equations until the stationary convection is reached. Then we produce the magnetic field generation and amplification by Biermann's battery seed and local dynamo. We

Lockman-SpReSO is a deep optical spectroscopic survey of a complete sample of galaxies previously observed at the greatest depth in X-ray, far infrared, and sub-millimeter, using, respectively, XMM-Newton, Spitzer, Herschel, and radio observations covering the central 24 x 24 arcmin 2 of the Lockman Hole field. The main scientific objective is to

Scientific data analysis pipelines commonly use high-level technologies that were popular when they were created, only providing an immediate solution which is unlikely to be sustainable or reproducible in the future. We have implemented "Maneage" (Managing data Lineage), a solution which stores the project in machine-actionable and human-readable