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

Abstract Mid-infrared (mid-IR) observations are powerful in identifying heavily obscured
active galactic nuclei (AGN) that have weak emission in other wavelengths. Data from the …

We present the first subarcsecond-resolution mid-infrared (MIR) atlas of local active galactic
nuclei (AGN). Our atlas contains 253 AGN with a median redshift of z= 0.016, and includes …

Type 2 active galactic nuclei (AGNs) show signatures of accretion onto a supermassive
black hole through strong, high-ionization, narrow emission lines extended on scales of …

We present results from a comprehensive survey of 70 radio galaxies at redshifts 1< z< 5.2
using the PACS and SPIRE instruments on board the Herschel Space Observatory …

We present results from model fitting to the spectral energy distribution (SED) of a
homogeneous sample of Seyfert II galaxies drawn from the 12 μm Galaxy Sample. Imaging …

ABSTRACT We present Multi-Unit Spectroscopic Explorer (MUSE) integral-field
spectroscopy of ESO 253− G003, which hosts a known active galactic nucleus (AGN) and …

We present the result of a systematic infrared 2.5–5 μm spectroscopic study of 22 nearby
infrared galaxies over a wide infrared luminosity range (10 10 L☉< L IR< 10 13 L☉) …

We present a 3D radiative transfer model for the spectral energy distribution (SED) of NGC
1365, which is a 'changing look'Seyfert 1.8 type active galactic nucleus (AGN). The SED …

We present the analysis of Chandra and NuSTAR spectra of NGC 4968, a local (D∼ 44
Mpc) 12 μm selected Seyfert 2 galaxy, enshrouded within Compton-thick layers of obscuring …