Mahony, E. K.E. K.MahonyMorganti, R.R.MorgantiPRANDONI, ISABELLAISABELLAPRANDONIvan Bemmel, I.I.van Bemmel2020-04-292020-04-2920160004-6337http://hdl.handle.net/20.500.12386/24316The Lockman Hole Project is a wide international collaboration aimed at exploiting the multi-band extensive and deep information available for the Lockman Hole region, with the aim of better characterizing the physical and evolutionary properties of the various source populations detected in deep radio fields. Recent observations with the LOw-Frequency ARray (LOFAR) extends the multi-frequency radio information currently available for the Lockman Hole (from 350 MHz up to 15 GHz) down to 150 MHz, allowing us to explore a new radio spectral window for the faint radio source population. These LOFAR observations allow us to study the population of sources with spectral peaks at lower radio frequencies, providing insight into the evolution of GPS and CSS sources. In this general framework, I present preliminary results from 150 MHz LOFAR observations of the Lockman Hole field. <P />STAMPAenArticle10.1002/asna.2015122792-s2.0-84959017097000370147600023https://onlinelibrary.wiley.com/doi/abs/10.1002/asna.2015122792016AN....337..135MFIS/05 - ASTRONOMIA E ASTROFISICAScienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation