The active galactic nucleus (AGN) phenomenon results from a supermassive black hole
accreting its surrounding gaseous and dusty material. The infrared (IR) regime provides …

We present the first results of the Galaxy Activity, Torus, and Outflow Survey (GATOS), a
project aimed at understanding the properties of the dusty molecular tori and their …

Observational studies of AGN in the mid-infrared regime are crucial to our understanding of
AGN and their role in the evolution of galaxies. Mid-IR-based selection of AGN is …

We study the relation between obscuration and supermassive black hole (SMBH) accretion
using a large sample of hard X-ray selected active galactic nuclei (AGNs). We find a strong …

We use JWST/MIRI MRS spectroscopy of a sample of six local obscured type 1.9/2 active
galactic nuclei (AGN) to compare their nuclear mid-IR absorption bands with the level of …

The ionisation cones of NGC 5728 have a deficit of molecular gas based on millimetre
observations of CO (2-1) emission. Although photoionisation from the active nucleus may …

Accreting supermassive black holes (SMBHs) located at the centers of galaxies are typically
surrounded by large quantities of gas and dust. The structure and evolution of this …

We present a UV to millimeter spectral energy distribution (SED) analysis of 16
hyperluminous, dust-obscured quasars at z∼ 3, selected by the Wide-field Infrared Survey …

We study the distribution of cold molecular gas in the circumunuclear disks (CND; r≤ 200
pc) of a sample of 64 nearby (DL= 7− 45 Mpc) disk galaxies–including 45 active galactic …

We present a statistical analysis of the properties of the obscuring material around active
galactic nuclei (AGN). This study represents the first of its kind for an ultra-hard X-ray (14 …