about
The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3.PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas FractionsCombined CO and dust scaling relations of depletion time and molecular gas fractions with cosmic time, specific star-formation rate, and stellar massThe molecular gas content of z = 3 Lyman break galaxies: evidence of a non-evolving gas fraction in main-sequence galaxies at z > 2Witnessing Galaxy Assembly at the Edge of the Reionization EpochA higher efficiency of converting gas to stars pushes galaxies at z ~ 1.6 well above the star-forming main sequenceFaint high-redshift AGN in theChandradeep field south: the evolution of the AGN luminosity function and black hole demographyObscured star formation and environment in the COSMOS fieldDEEPSPITZER24 μm COSMOS IMAGING. I. THE EVOLUTION OF LUMINOUS DUSTY GALAXIES—CONFRONTING THE MODELSChasing highly obscured QSOs in the COSMOS fieldPassive galaxies as tracers of cluster environments atz~ 2Spectroscopic identifications of Spitzer sources in the SWIRE/XMM-Newton/ELAIS-S1 field: a large fraction of active galactic nucleus with high F(24 {mu}m)/F(R) ratioThe ESO-Spitzer Imaging extragalactic Survey (ESIS) II. VIMOS I, z wide field imaging of ELAIS-S1 and selection of distant massive galaxiesThe XMM-Newton survey of the ELAIS-S1 fieldUnveiling Obscured Accretion in the Chandra Deep Field–SouthThe XMM-Newton survey of the ELAIS-S1 fieldIn and out star formation inz ~ 1.5 quiescent galaxies from rest-frame UV spectroscopy and the far-infraredA direct constraint on the gas content of a massive, passively evolving elliptical galaxy at z = 1.43Evidence for feedback in action from the molecular gas content in thez~ 1.6 outflowing QSO XID2028Gas reservoir of a hyper-luminous quasar atz= 2.6Discovery of strong iron k{alpha} emitting Compton thick quasars at z = 2.5 and 2.9Ionised outflows inz~ 2.4 quasar host galaxiesThe HELLAS2XMM surveyThe HELLAS2XMM Survey. VII. The Hard X‐Ray Luminosity Function of AGNs up toz= 4: More Absorbed AGNs at Low Luminosities and High Redshifts(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxiesMillimeter imaging of submillimeter galaxies in the COSMOS field: redshift distributionThe MAGNUM survey: positive feedback in the nuclear region of NGC 5643 suggested by MUSEOn the nature of the absorber in IRAS 09104+4109: the X-ray and mid-infrared viewEvidence of strong quasar feedback in the early UniverseSuzaku reveals X-ray continuum piercing the nuclear absorber in Markarian 231AGN wind scaling relations and the co-evolution of black holes and galaxiesBlowin' in the wind: both "negative" and "positive" feedback in an obscured high-z quasarThe hidden quasar nucleus of a WISE-selected, hyperluminous, dust-obscured galaxy atz~ 2.3The multi-phase winds of Markarian 231: from the hot, nuclear, ultra-fast wind to the galaxy-scale, molecular outflowVery extended cold gas, star formation and outflows in the halo of a bright quasar atz> 6Massive molecular outflows and evidence for AGN feedback from CO observationsHigh resolution mapping of CO(1–0) in NGC 6240NGC 6240: extended CO structures and their association with shocked gasThe physics and the structure of the quasar-driven outflow in Mrk 231Quasar feedback revealed by giant molecular outflows
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description
hulumtuese
@sq
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
C Feruglio
@nl
Chiara Feruglio
@en
Chiara Feruglio
@es
type
label
C Feruglio
@nl
Chiara Feruglio
@en
Chiara Feruglio
@es
altLabel
C Feruglio
@en
prefLabel
C Feruglio
@nl
Chiara Feruglio
@en
Chiara Feruglio
@es
P106
P1153
24586900600
P21
P31
P496
0000-0002-4227-6035