most citedSUPER VII. Morphology and kinematics of H emission in AGN host galaxies at Cosmic noon using SINFONI

16 citations · 29 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2024

Unveiling the (in)consistencies among the galaxy stellar mass function, star formation histories, satellite abundances and intracluster light from a semi-empirical perspective

Hao Fu, Francesco Shankar, Mohammadreza Ayromlou +16

In a hierarchical, dark matter-dominated Universe, stellar mass functions (SMFs), galaxy merger rates, star formation histories (SFHs), satellite abundances, and intracluster light…

cond-mat.stat-mech20247 cited

Thermodynamic precision of a chain of motors: the difference between phase and noise correlation

Giulio Costantini, Andrea Puglisi

Inspired by recent experiments on fluctuations of the flagellar beating in sperms and C. reinhardtii, we investigate the precision of phase fluctuations in a system of nearest-neig…

astro-ph.GA20238 cited

Probing the roles of orientation and multi-scale gas distributions in shaping the obscuration of Active Galactic Nuclei through cosmic time

Alba V. Alonso-Tetilla, Francesco Shankar, Fabio Fontanot +14

The origin of obscuration in Active Galactic Nuclei (AGN) is still an open debate. In particular, it is unclear what drives the relative contributions to the line-of-sight column d…

astro-ph.GA2023

Obscuration beyond the nucleus: infrared quasars can be buried in extreme compact starbursts

Carolina Andonie, David M. Alexander, Claire Greenwell +14

In the standard quasar model, the accretion disk obscuration is due to the canonical dusty torus. Here, we argue that a substantial part of the quasar obscuration can come from the…

astro-ph.GA202316 cited

SUPER VII. Morphology and kinematics of H emission in AGN host galaxies at Cosmic noon using SINFONI

D. Kakkad, V. Mainieri, G. Vietri +19

We present spatially resolved H properties of 21 type 1 AGN host galaxies at z2 derived from the SUPER survey. These targets were observed with the adaptive optics capabil…

astro-ph.GA202113 cited

Differential attenuation in star-forming galaxies at 0.3 1.5 in the SHARDS/CANDELS field

L. Rodríguez-Muñoz, G. Rodighiero, P. G. Pérez-González +21

We use a sample of 706 galaxies, selected as [OII]3727 ([OII]) emitters in the Survey for High- Absorption Red and Dead Sources (SHARDS) on the CANDELS/GOODS-N field, to stud…