The OSIRIS Tunable Emission Line Object survey (OTELO) will provide a deep, complete sample of active galactic nuclei (AGN), and able to separate them...
AGN-host galaxy connection: morphology and colours of X-ray selected AGN at z ≤ 2
Context. The connection between active galactic nuclei (AGN) and their host galaxies has been widely studied and found to be of great importance for providing...
The connection between active galactic nuclei (AGN) and their hosts showed to be important for understanding the formation and evolution of active galaxies...
We present the most complete atlas of nuclear rings to date. We include 113 rings found in 107 galaxies, six of which are elliptical galaxies, five are highly...
The Advanced Large Homogeneous Area Medium Band Redshift Astronomical (ALHAMBRA) survey is a photometric survey designed to study systematically cosmic...
ALMA High-Level Data Products: submillimetre counterparts of SDSS quasars in the ALMA footprint
The Atacama Large Millimetre/submillimetre Array (ALMA) is the world's most advanced radio interferometric facility, producing science data with an average rate...
ALMA images the many faces of the <ASTROBJ>NGC 1068</ASTROBJ> torus and its surroundings
Aims: We investigate the fueling and the feedback of nuclear activity in the nearby (D = 14 Mpc) Seyfert 2 barred galaxy NGC 1068 by studying the distribution...
ALMA imaging of C2H emission in the disk of NGC 1068
Aims: We study the feedback of star formation and nuclear activity on the chemistry of molecular gas in NGC 1068, a nearby (D = 14 Mpc) Seyfert 2 barred galaxy...
ALMA Observations of Lyα Blob 1: Halo Substructure Illuminated from Within
We present new Atacama Large Millimeter/Submillimeter Array (ALMA) 850 μm continuum observations of the original Lyα Blob (LAB) in the SSA22 field at z = 3.1...