605 citations · 13.7k across the 314 of their papers we have counts for
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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…
MAGNUM survey: Compact jets causing large turmoil in galaxies -- Enhanced line widths perpendicular to radio jets as tracers of jet-ISM interaction
G. Venturi, G. Cresci, A. Marconi +10
Outflows accelerated by AGN are commonly observed in the form of coherent, mildly collimated high-velocity gas directed along the AGN ionisation cones and kinetically powerful (>$1…
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…
Constraints on the [CII] luminosity of a proto-globular cluster at z~6 obtained with ALMA
F. Calura, E. Vanzella, S. Carniani +11
We report on ALMA observations of D1, a system at z~6.15 with stellar mass M_* ~ 10^7 M_sun containing globular cluster (GC) precursors, strongly magnified by the galaxy cluster MA…
The WISSH QSOs project IX. Cold gas content and environment of luminous QSOs at z~2.4-4.7
M. Bischetti, C. Feruglio, E. Piconcelli +23
Sources at the brightest end of QSO luminosity function during the peak epoch of star formation and black hole accretion (z~2-4, i.e. Cosmic noon) are privileged sites to study the…
Galaxy-scale ionised winds driven by ultra-fast outflows in two nearby quasars
A. Marasco, G. Cresci, E. Nardini +14
We use MUSE adaptive optics (AO) data in Narrow Field Mode to study the properties of the ionised gas in MR 2251-178 and PG 1126-041, two nearby (z~0.06) bright quasars hosting sub…
Velocity dispersion in the interstellar medium of early galaxies
M. Kohandel, A. Pallottini, A. Ferrara +5
We study the structure of spatially resolved, line-of-sight velocity dispersion for galaxies in the Epoch of Reionization (EoR) traced by [CII] line emission. Our labo…
Early galaxy growth: mergers or gravitational instability?
A. Zanella, A. Pallottini, A. Ferrara +4
We investigate the spatially-resolved morphology of galaxies in the early Universe. We consider a typical redshift z = 6 Lyman Break galaxy, "Althaea" from the SERRA hydrodynamical…
Gas and Star Formation from HD and Dust Emission in a Strongly Lensed Galaxy
Gareth C. Jones, Roberto Maiolino, Paola Caselli +1
The molecular gas content of high-redshift galaxies is a highly sought-after property. However, H is not directly observable in most environments, so its mass is probed through…
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…
What Drives Galaxy Quenching? Resolving Molecular Gas and Star Formation in the Green Valley
Simcha Brownson, Francesco Belfiore, Roberto Maiolino +2
We study quenching in seven green valley galaxies on kpc scales by resolving their molecular gas content using \textsuperscript{12}CO(1-0) observations obtained with NOEMA and ALMA…
Properties of the Multiphase Outflows in Local (Ultra)luminous Infrared Galaxies
A. Fluetsch, R. Maiolino, S. Carniani +14
Galactic outflows are known to consist of several gas phases, however, so far the connection between these multiple phases has been investigated little and only in a few objects. I…
Missing [CII] emission from early galaxies
S. Carniani, A. Ferrara, R. Maiolino +9
ALMA observations have revealed that [CII] 158m line emission in high-z galaxies is ~2-3 more extended than the UV continuum emission. Here we explore whether surface br…
The ALPINE-ALMA [CII] Survey: CGM pollution and gas mixing by tidal stripping in a merging system at z~4.57
M. Ginolfi, G. C. Jones, M. Bethermin +25
We present ALMA observations of a merging system at z ~ 4.57, observed as a part of the ALMA Large Program to INvestigate [CII] at Early times (ALPINE) survey. Combining ALMA [CII]…
Warm dust in high-z galaxies: origin and implications
L. Sommovigo, A. Ferrara, A. Pallottini +3
ALMA observations have revealed the presence of dust in galaxies in the Epoch of Reionization (redshift ). However, the dust temperature, , remains unconstrained, and thi…
Predicting FIR lines from simulated galaxies
Alessandro Lupi, Andrea Pallottini, Andrea Ferrara +3
Far-infrared (FIR) emission lines are a powerful tool to investigate the properties of the interstellar medium, especially in high-redshift galaxies, where ALMA observations have p…
Star formation law in the EoR from [CII] and CIII] lines
L. Vallini, A. Ferrara, A. Pallottini +2
We present a novel method to simultaneously characterise the star formation law and the interstellar medium properties of galaxies in the Epoch of Reionization (EoR) through the co…
The ALMA view of the high-redshift relation between supermassive black holes and their host galaxies
A. Pensabene, S. Carniani, M. Perna +4
This work aims at studying the relation of a sample of quasars by constraining their host galaxy masses through full kinematical modeling of the cold gas k…
Difficulties in Mid-Infrared selection of AGN in dwarf galaxies
Alessandro Lupi, Tullia Sbarrato, Stefano Carniani
While massive black holes (MBHs) are known to inhabit all massive galaxies, their ubiquitous presence in dwarf galaxies has not been confirmed yet, with only a limited number of so…