papers

Publications (23)

astro-ph.GA2020

The Ionised- and Cool-Gas Content of The BR1202-0725 System as seen by MUSE and ALMA

A. B. Drake, F. Walter, M. Novak +7

We present MUSE observations of the gas-rich major-merger BR1202-0725 at z~4.7, which constitutes one of the most overdense fields known in the early Universe. We utilise these dat…

astro-ph.GA2025

Revised optical classification of a sample of gamma-ray emitting AGN with GTC and VLT

B. Dalla Barba, L. Foschini, M. Berton +10

We report the results of the optical follow-up of a sample of -ray-emitting active galactic nuclei (AGN). New high-quality optical spectra were obtained using Gran Telescopio C…

astro-ph.GA2016

The Pan-STARRS1 distant z>5.6 quasar survey: more than 100 quasars within the first Gyr of the universe

E. Bañados, B. P. Venemans, R. Decarli +33

Luminous quasars at z>5.6 can be studied in detail with the current generation of telescopes and provide us with unique information on the first gigayear of the universe. Thus far…

astro-ph.GA2015

The identification of z-dropouts in Pan-STARRS1: three quasars at 6.5<z<6.7

B. P. Venemans, E. Bañados, R. Decarli +30

Luminous distant quasars are unique probes of the high redshift intergalactic medium (IGM) and of the growth of massive galaxies and black holes in the early universe. Absorption d…

astro-ph.GA2023

Powerful Radio Sources in the Southern Sky. II. A SWIFT X-Ray Perspective

F. Massaro, S. V. White, A. Paggi +18

We recently constructed the G4Jy-3CRE, a catalog of extragalactic radio sources based on the GLEAM 4-Jy (G4Jy) sample, with the aim of increasing the number of powerful radio galax…

astro-ph.GA2022

The cavity of 3CR 196.1: H emission spatially associated with an X-ray cavity

A. Jimenez-Gallardo, E. Sani, F. Ricci +20

We present a multifrequency analysis of the radio galaxy 3CR 196.1 (), associated with the brightest galaxy of the cool core cluster CIZAJ0815.4-0303. This nearby radio…

astro-ph.GA2018

An 800-million-solar-mass black hole in a significantly neutral Universe at redshift 7.5

E. Bañados, B. P. Venemans, C. Mazzucchelli +15

Quasars are the most luminous non-transient objects known and as a result they enable studies of the Universe at the earliest cosmic epochs. Despite extensive efforts, however, the…

astro-ph.GA2021

Raining in MKW 3s: a Chandra-MUSE analysis of X-ray cold filaments around 3CR 318.1

A. Jimenez-Gallardo, F. Massaro, B. Balmaverde +23

We present the analysis of X-ray and optical observations of gas filaments observed in the radio source 3CR 318.1, associated with NGC 5920, the Brightest Cluster Galaxy (BCG) of M…

astro-ph.GA2018

Chandra X-rays from the redshift 7.54 quasar ULAS J1342+0928

E. Bañados, T. Connor, D. Stern +9

We present a 45 ks Chandra observation of the quasar ULAS J1342+0928 at z=7.54. We detect 14.0^{+4.8}_{-3.7} counts from the quasar in the observed-frame energy range 0.5-7.0 keV (…

astro-ph.GA2023

Powerful Radio Sources in the Southern Sky. I. Optical Identifications

F. Massaro, S. V. White, A. Garcia-Perez +18

Since the early sixties, our view of radio galaxies and quasars has been drastically shaped by discoveries made thanks to observations of radio sources listed in the Third Cambridg…

astro-ph.GA2019

Spectral Energy Distributions of Companion Galaxies to z6 Quasars

C. Mazzucchelli, R. Decarli, E. P. Farina +10

Massive, quiescent galaxies are already observed at redshift , i.e. 1.5 Gyr after the Big Bang. Current models predict them to be formed via massive, gas-rich mergers…

astro-ph.GA2024

A lack of LAEs within 5Mpc of a luminous quasar in an overdensity at z=6.9: potential evidence of quasar negative feedback at protocluster scales

Trystan S. Lambert, R. J. Assef, C. Mazzucchelli +13

High-redshift quasars are thought to live in the densest regions of space which should be made evident by an overdensity of galaxies around them. However, campaigns to identify the…

astro-ph.GA2026

VAR-PZ: Constraining the Photometric Redshifts of Quasars using Variability

S. Satheesh-Sheeba, R. J. Assef, T. Anguita +33

The Vera C. Rubin Observatory LSST is expected to discover tens of millions of new Active Galactic Nuclei (AGNs). The survey's exceptional cadence and sensitivity will enable UV/op…

astro-ph.GA2024

The host galaxies of radio-loud quasars at z>5 with ALMA

C. Mazzucchelli, R. Decarli, S. Belladitta +13

The interaction between radio-jets and quasar host galaxies plays a paramount role in quasar/galaxy co-evolution. However, very little has been known so far about this interaction…

astro-ph.GA2023

XQR-30: Black Hole Masses and Accretion Rates of 42 z>6 Quasars

C. Mazzucchelli, M. Bischetti, V. D'Odorico +19

We present bolometric luminosities, black hole masses and Eddington ratios for 42 luminous quasars at z>6 using high signal-to-noise ratio VLT/X-Shooter spectra, acquired in the en…

astro-ph.GA2016

No overdensity of Lyman Alpha Emitting Galaxies around a quasar at z~5.7

C. Mazzucchelli, E. Bañados, R. Decarli +4

Bright quasars, observed when the Universe was less than one billion years old (z>5.5), are known to host massive black holes (~10 M), and are thought to reside in…

astro-ph.GA2025

How similar are narrow-line Seyfert 1 galaxies and high-z type 1 AGN?

M. Berton, E. Järvelä, A. Tortosa +1

The recent observations of highly accreting supermassive black holes (SMBH) at very high redshift (4) with the James Webb Space Telescope (JWST) allowed us to shed light for the…

astro-ph.GA2026

VAR-PZnn: A machine-learning framework for AGN photometric redshifts using color and variability-based features

S. Satheesh-Sheeba, P. Sánchez-Sáez, R. J. Assef +39

Photometric redshift estimation for active galactic nuclei (AGNs) remains a fundamental challenge for current and upcoming large-scale photometric surveys. Traditional spectral ene…

astro-ph.GA2023

XQR-30: the ultimate XSHOOTER quasar sample at the reionization epoch

Valentina D'Odorico, E. Banados, G. D. Becker +46

The final phase of the reionization process can be probed by rest-frame UV absorption spectra of quasars at z>6, shedding light on the properties of the diffuse intergalactic mediu…

astro-ph.GA2022

Widespread, strong outflows in XQR-30 quasars at the Reionisation epoch

M. Bischetti, C. Feruglio, V. D'Odorico +23

Luminous quasars powered by accretion onto billion solar mass black holes already exist at the epoch of Reionisation, when the Universe was 0.5-1 Gyr old. These objects likely resi…

astro-ph.GA2017

Physical properties of 15 quasars at

C. Mazzucchelli, E. Bañados, B. P. Venemans +21

Quasars are galaxies hosting accreting supermassive black holes; due to their brightness, they are unique probes of the early universe. To date, only few quasars have been reported…

astro-ph.GA2026

4MOST ChANGES: Catalog of high-redshift quasar candidates (4.5 < < 7) selected with SED fitting

T. Mkrtchyan, C. Mazzucchelli, R. J. Assef +12

The identification of high-redshift quasars () is critical for studying the early Universe, supermassive black hole growth, and cosmic reionization. Most known high-redshi…

astro-ph.GA2021

An ALMA multi-line survey of the ISM in two quasar host-companion galaxy pairs at

A. Pensabene, R. Decarli, E. Bañados +15

We present a multi-line survey of the interstellar medium (ISM) in two quasar (QSO) host galaxies, PJ231-20 () and PJ308-21 (), and their two companion galaxi…