activity
20162022
most citedPrevalence of radio jets associated with galactic outflows and feedback from quasars

169 citations · 991 across the 20 of their papers we have counts for

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Showing 2020Show all

8 papers · 1 filter

astro-ph.GA202042 cited

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…

astro-ph.GA2020

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…

astro-ph.GA2020

The Evolution of Gas-Phase Metallicity and Resolved Abundances in Star-forming Galaxies at

S. Gillman, A. L. Tiley, A. M. Swinbank +10

We present an analysis of the chemical abundance properties of 650 star-forming galaxies at . Using integral-field observations from the -band Multi-O…

astro-ph.GA2020

Probing the origin of low-frequency radio emission in PG quasars with the uGMRT -- I

Silpa S., P. Kharb, L. C. Ho +3

We present the results from 685 MHz observations with the upgraded Giant Metrewave Radio Telescope (uGMRT) of 22 quasars belonging to the Palomar-Green (PG) quasar sample. Only fou…

astro-ph.GA2020

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…

astro-ph.GA2020

Flat Rotation Curves of Star-Forming Galaxies and Evidence of Disk-Scale Length Evolution

Gauri Sharma, Paolo Salucci, C. M. Harrison +2

We investigate the shape of the Rotation Curves (RCs) of star-forming galaxies and compare them with the local star-forming galaxies. For this purpose, we have used