We exploit the unprecedented depth of integral field data from the KMOS Ultra-deep
Rotational Velocity Survey (KURVS) to analyse the strong (Hα) and forbidden ([N ii],[S ii]) …

This is the second paper in a series using data from tens of thousands S0 galaxies of the
local Universe (z≲ 0.1) retrieved from the NASA-Sloan Atlas. It builds on the outcomes of the …

For spiral galaxies, the active galactic nucleus (AGN) and some physical parameters that
concern the host galaxy such as spiral arm radius and density can play an important role in …

We study the host properties and environment of active galactic nuclei (AGNs) galaxies,
taken from SDSS-DR12, across the [O iii]/H β versus [N ii]/H α diagnostic diagram. We select …

The coevolution between supermassive black holes (SMBHs) and their host galaxies has
been proposed for more than a decade, albeit with little direct evidence about black hole …

Our understanding of galaxy evolution is often hindered by the complexity of the processes
that drive it. Star formation offers a powerful tool for tracing galaxy growth, and star formation …

In this paper we summarise the research that is currently going on in Ethiopia and East-
Africa in extragalactic astronomy and physics of active galaxies and active galactic nuclei …

In this work, we study the properties of galaxies that are showing the inside-out assembly
(which we call inside-out assembled galaxies; IOAGs), with the main aim to understand …