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The First Integral Field Unit Spectroscopic View of Shocked Cluster Galaxies
Andra Stroe, Maryam Hussaini, Bernd Husemann +2
Galaxy clusters grow by merging with other clusters, giving rise to Mpc-wide shock waves that travel at 1000-2500 km/s through the intra-cluster medium. To study the effects of mer…
SUPER IV. CO(J=3-2) properties of active galactic nucleus hosts at cosmic noon revealed by ALMA
C. Circosta, V. Mainieri, I. Lamperti +23
Feedback from AGN is thought to be key in shaping the life cycle of their host galaxies by regulating star-formation activity. Therefore, to understand the impact of AGN on star fo…
SUPER III. Broad Line Region properties of AGN at z2
G. Vietri, V. Mainieri, D. Kakkad +27
The SINFONI survey for Unveiling the Physics and Effect of Radiative feedback (SUPER) was designed to conduct a blind search for AGN-driven outflows on X-ray selected AGN at redshi…
A significant excess in major merger rate for AGNs with the highest Eddington ratios at z<0.2
V. Marian, K. Jahnke, I. Andika +16
Observational studies are increasingly finding evidence against major mergers being the dominant mechanism responsible for triggering AGN. After studying the connection between maj…
The stellar metallicity distribution function of galaxies in the CALIFA survey
A. Mejía-Narváez, S. F. Sánchez, E. A. D. Lacerda +4
We present a novel method to retrieve the chemical structure of galaxies using integral field spectroscopy data through the stellar Metallicity Distribution Function (MDF). This is…
SUPER-II: Spatially resolved ionized gas kinematics and scaling relations in z~2 AGN host galaxies
D. Kakkad, V. Mainieri, G. Vietri +27
The SINFONI survey for Unveiling the Physics and Effect of Radiative feedback (SUPER) aims at tracing and characterizing ionized gas outflows and their impact on star formation in…