We explore the properties of the host galaxies of X-ray selected AGN in the COSMOS field
using the Chandra Legacy sample and the LEGA-C survey VLT optical spectra. Our main …

It is still a matter of intense debate how supermassive black holes (SMBHs) grow and the
role played by feedback from active galactic nuclei (AGN) in the coevolution of SMBHs and …

It is well known that supermassive black holes (SMBHs) and their host galaxies undergo a
process of co-evolution. Feedback from active galactic nuclei (AGNs) plays an important role …

We present the identification and analysis of an X-ray selected AGN sample that lie within
the local (z< 0.35) galaxy population. From a parent sample of 22 079 MPA-JHU (based on …

We present an improved study of the relation between supermassive black hole growth and
their host galaxy properties in the local Universe (z< 0.33). To this end, we build an …

In this work, we study the relation of the cosmic environment and morphology with the star
formation and stellar population of galaxies. Most importantly, we examine if this relation …

We used active galactic nuclei (AGNs) with X-ray luminosities, LX, 2− 10 keV∼ 10 42.5− 44
erg s− 1, from the COSMOS-Legacy survey that lie within the UltraVISTA region and cross …

This study involves a comparative analysis of the star formation rates (SFRs) of active
galactic nucleus (AGN) galaxies and non-AGN galaxies and of the SFRs of type 1 and 2 …

In this work, we compare the supermassive black hole (SMBH) and host galaxy properties of
X-ray obscured and unobscured AGN. For that purpose, we used∼ 35 000 X-ray detected …

The X-ray luminosity function (XLF) of active galactic nuclei (AGN) offers a robust tool to
study the evolution and the growth of the supermassive black-hole population over cosmic …