Regional Science and Technology Fund
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Esta é uma presença online oficial do Governo dos Açores
Objective
In this project we aim to explore state-of-the-art galaxy and SMBH evolution models, implementing improved recipes for radio emission, and compare the results to the known population of powerful AGN, as seen at radio frequencies.
We will also implement a monitoring program of nearby AGN, using the Santa Maria radio telescope, part of the RAEGE network. This will complement the above approach, by setting the framework to further explore the physical mechanisms behind AGN radio emission, as revealed by AGN variability.
Results & Impact
With the implementation of the aforementioned approaches, we will:
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