activity
19932026
most citedMass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

2k citations · 28k across the 222 of their papers we have counts for

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74 papers · 1 filter

astro-ph.GA2026

Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys

Giovanni Mazzolari, Dharam V. Lal, Isabella Prandoni +6

The advent of JWST has revealed a large population of AGN at , which are dex more abundant than previously expected, including also the enigmatic population of Little…

astro-ph.GA2026

No evolution in the number density of little red dots from cosmic dawn to cosmic noon

Federica Loiacono, Roberto Gilli, Marco Mignoli +24

We present our search for little red dots (LRDs) in the "J1030 field", a region of the sky around the quasar SDSS J1030+0524, observed by the JWST EIGER program. Over 1…

astro-ph.GA2026

Radio selection of heavily obscured AGN in the J1030 field: unraveling a missing Compton-thick population

Giovanni Mazzolari, Roberto Gilli, Marco Mignoli +21

We tested the effectiveness of radio selection to discover heavily obscured AGNs, particularly at high-z, and we measured their abundance for the first time from a radio perspectiv…

astro-ph.GA2025

Tracing AGN-Galaxy Co-Evolution with UV Line-Selected Obscured AGN

Luigi Barchiesi, Lucia Marchetti, Mattia Vaccari +11

Understanding black hole-galaxy co-evolution and the role of AGN feedback requires complete AGN samples, including heavily obscured systems. In this work, we present the first UV l…

astro-ph.GA2025★ 10 cited

A big red dot at cosmic noon

Federica Loiacono, Roberto Gilli, Marco Mignoli +22

We report the discovery of a little red dot (LRD), dubbed BiRD ('big red dot'), at in the field around the quasar SDSSJ1030+0524. Using NIRCam images, we identifie…

astro-ph.GA2025★ 1 cited

Intervening nuclear obscuration changing the X-ray look of the QSO CFHQS J164121+375520

Fabio Vito, William Nielsen Brandt, Andrea Comastri +16

X-ray observations of the optically selected QSO CFHQS J164121+375520 (hereafter J1641) revealed that its flux dropped by a factor from 2018, when it was a bri…

astro-ph.GA2024★ 18 cited

The radio properties of the JWST-discovered AGN

G. Mazzolari, R. Gilli, R. Maiolino +23

We explore the radio emission of JWST-selected Broad Line AGN (BLAGN, or type 1) in the GOODS-N field. We use deep radio data at different frequencies (144\,MHz, 1.5\,GHz, 3\,GHz,…

astro-ph.GA2024★ 27 cited

Narrow line AGN selection in CEERS: spectroscopic selection, physical properties, X-ray and radio analysis

Giovanni Mazzolari, Jan Scholtz, Roberto Maiolino +11

In this work, we spectroscopically select narrow-line AGNs (NLAGNs) among the ~300 publicly available medium-resolution spectra of the Cosmic Evolution Early Release Science Survey…

astro-ph.GA2024★ 18 cited

Extreme Ionizing Properties of Metal-Poor, Muv ~ -12 Star Complex in the first Gyr

E. Vanzella, F. Loiacono, M. Messa +38

We report the serendipitous discovery of a faint (M_UV > -12.2), low-metallicity (Z ~ 0.02 Zsun), ionizing source (dubbed T2c) with a spectroscopic redshift of z=6.146. T2c is part…

astro-ph.GA2024★ 26 cited

A quasar-galaxy merger at : rapid host growth via accretion of two massive satellite galaxies

Roberto Decarli, Federica Loiacono, Emanuele Paolo Farina +38

We present JWST/NIRSpec Integral Field Spectroscopy in the rest-frame optical bands of the system PJ308-21, a quasar at caught as its host galaxy interacts with companio…

astro-ph.GA2024★ 7 cited

Euclid preparation. Observational expectations for redshift z<7 active galactic nuclei in the Euclid Wide and Deep surveys

Euclid Collaboration, M. Selwood, S. Fotopoulou +260

We forecast the expected population of active galactic nuclei (AGN) observable in the Euclid Wide Survey (EWS) and Euclid Deep Survey (EDS). Starting from an X-ray luminosity funct…

astro-ph.GA2024★ 66 cited

New AGN diagnostic diagrams based on the [OIII] auroral line

G. Mazzolari, H. Übler, R. Maiolino +8

The James Webb Space Telescope (JWST) is revolutionizing our understanding of black holes formation and growth in the early Universe. However, JWST has also revealed that some of t…

astro-ph.GA2024★ 8 cited

COSMOS2020: Investigating the AGN-obscured accretion phase at via [NeV] selection

L. Barchiesi, C. Vignali, F. Pozzi +7

We investigated the properties of 94 [NeV]3426AA-selected type 2 AGN in COSMOS at z=0.6-1.2, performing optical-to-far-infrared spectral energy distribution fitting. In addition, w…

astro-ph.GA2024★ 34 cited

A quasar-galaxy merger at : black hole mass and quasar properties from the NIRSpec spectrum

Federica Loiacono, Roberto Decarli, Marco Mignoli +31

We present JWST/NIRSpec integral field data of the quasar PJ308-21 at . As shown by previous ALMA and HST imaging, the quasar has two companion sources, interacting with…

astro-ph.GA2024★ 15 cited

Heavily Obscured AGN detection: a Radio vs X-ray challenge

Giovanni Mazzolari, Roberto Gilli, Marcella Brusa +11

In this work, we study the AGN radio detection effectiveness in the major deep extragalactic surveys, considering different AGN obscuration levels, redshift, and AGN bolometric lum…

astro-ph.GA2023

Euclid preparation. Spectroscopy of active galactic nuclei with NISP

Euclid Collaboration, E. Lusso, S. Fotopoulou +246

The statistical distribution and evolution of key properties (e.g. accretion rate, mass, or spin) of active galactic nuclei (AGN), remain an open debate in astrophysics. The ESA Eu…

astro-ph.GA2023★ 18 cited

The VANDELS ESO public spectroscopic survey: The spectroscopic measurements catalogue

M. Talia, C. Schreiber, B. Garilli +36

VANDELS is a deep spectroscopic survey, performed with the VIMOS instrument at VLT, aimed at studying in detail the physical properties of high-redshift galaxies. VANDELS targeted…

astro-ph.GA2023★ 6 cited

Identifying Lyα emitter candidates with Random Forest: learning from galaxies in CANDELS survey

L. Napolitano, L. Pentericci, A. Calabrò +8

The physical processes which make a galaxy a Lyman Alpha Emitter have been extensively studied for the past 25 years. However, the correlations between physical and morphological p…

astro-ph.GA2023★ 74 cited

An extremely metal poor star complex in the reionization era: Approaching Population III stars with JWST

E. Vanzella, F. Loiacono, P. Bergamini +31

We present JWST/NIRSpec integral field spectroscopy (IFS) of a lensed Population III candidate stellar complex (dubbed Lensed And Pristine 1, LAP1), with a lensing-corrected stella…

astro-ph.GA2023★ 25 cited

The ionizing photon production efficiency of bright z2-5 galaxies

M. Castellano, D. Belfiori, L. Pentericci +27

We investigate the production efficiency of ionizing photons () of 1174 galaxies with secure redshift at z=2-5 from the VANDELS survey to determine the relation between…

astro-ph.GA2023★ 3 cited

LBT-MODS spectroscopy of high-redshift candidates in the Chandra J1030 field. A newly discovered z2.8 large scale structure

Stefano Marchesi, Marco Mignoli, Roberto Gilli +13

We present the results of a spectroscopic campaign with the Multi-Object Double Spectrograph (MODS) instrument mounted on the Large Binocular Telescope (LBT), aimed at obtaining a…

astro-ph.GA2023★ 7 cited

AGN feedback in an infant galaxy cluster: the LOFAR-Chandra view of the giant FRII radio galaxy J103025+052430 at z=1.7

M. Brienza, R. Gilli, I. Prandoni +19

In the nearby universe jets from AGN are observed to have a dramatic impact on their surrounding extragalactic environment. Their effect at the `cosmic noon' (z>1.5), the epoch whe…

astro-ph.GA2023★ 33 cited

Optical and mid-infrared line emission in nearby Seyfert galaxies

A. Feltre, C. Gruppioni, L. Marchetti +24

Line ratio diagnostics provide valuable clues on the source of ionizing radiation in galaxies with intense black hole accretion and starbursting events, such as local Seyfert or ga…

astro-ph.GA2022★ 15 cited

A deep 1.4 GHz survey of the J1030 equatorial field: a new window on radio source populations across cosmic time

Q. D'Amato, I. Prandoni, R. Gilli +12

We present deep L-Band observations of the equatorial field centered on the z=6.3 SDSS QSO, reaching a 1 sigma sensitivity of ~2.5 uJy at the center of the field. We extracted a ca…