Studies on slow radio transients
Aleksandra Wo{\l}owska, Magdalena Kunert-Bajraszewska, Kunal Mooley,, Aneta Siemiginowska, Preeti Kharb, C. H. Ishwara-Chandra, Gregg Hallinan,, Mariusz Gromadzki, Dorota Kozie{\l}-Wierzbowska

TL;DR
This paper reviews extensive studies of active galactic nuclei transitioning to radio-loud states, highlighting their diverse properties and introducing a new project to investigate slow radio transients.
Contribution
It provides a comprehensive overview of AGNs evolving into radio-loud states and proposes a novel observational project focused on slow radio transients.
Findings
Diverse physical parameters among studied AGNs.
Identification of gigahertz-peaked spectrum objects with rapid changes.
Introduction of a new observational approach for slow radio transients.
Abstract
We present a brief overview of a very extensive studies of the group of active galactic nuclei (AGNs) that transitioned to radio-loud state over the past few decades. The sample consists of twelve sources, both quasars and galaxies, showing the characteristics of gigahertz-peaked spectrum (GPS) objects undergoing relatively rapid changes, due to the evolution of their newly-born radio jets. Discussed objects also show a wide range of physical parameters such as bolometric luminosity, black hole mass and jet power, suggesting a great diversity among young active galactic nuclei and their hosts. Furthermore, we introduce a new observational project, the aim of which will be to investigate and gain a more in-depth understanding of the phenomenon of slow radio transients.
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