CORDIS Project
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This project aims to identify high redshift blazar candidates using Machine Learning techniques and multifrequency data. By focusing on the Damping Wing Pattern, it seeks to enhance our understanding of supermassive black holes and their role in the early Universe, particularly during the Epoch of Reionization.
Early Super Massive Black Holes (SMBH) continuously push our understanding of the formation of galaxies and structures in the Universe. SMBH accreting matter under the radio/jet mode produces powerful relativistic jets and emit beamed non-thermal radiation from radio up to very high energy gamma-rays.
Those jets pointing directly to Earth create the so-called Blazar phenomena, where the source appears exceptionally bright due to relativistic magnification (beaming) effects.
We can spot Blazars u…
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