about
Cosmological test with the QSO Hubble diagramGOODS-Herschel: ultra-deep XMM-Newton observations reveal AGN/star-formation connectionBlack hole accretion and host galaxies of obscured quasars in XMM-COSMOSThe XMM-Newton wide-field survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous active galactic nucleiThe X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOSOn the cosmic evolution of the scaling relations between black holes and their host galaxies: broad-line active galactic nuclei in the zCOSMOS surveyAGNfitter: A BAYESIAN MCMC APPROACH TO FITTING SPECTRAL ENERGY DISTRIBUTIONS OF AGNsFitting Spectral Energy Distributions of AGN A Markov Chain Monte Carlo ApproachThe nature of massive black hole binary candidates – II. Spectral energy distribution atlasThe nature of massive black hole binary candidates – I. Spectral properties and evolutionERRATUM: “THE OBSCURED FRACTION OF ACTIVE GALACTIC NUCLEI IN THE XMM-COSMOS SURVEY: A SPECTRAL ENERGY DISTRIBUTION PERSPECTIVE” (2013, ApJ, 777, 86)The incidence of obscuration in active galactic nucleiThe obscured fraction of active galactic nuclei in the XMM-COSMOS survey: a spectral energy distribution perspectiveA statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveysThe bolometric output and host-galaxy properties of obscured AGN in the XMM-COSMOS surveyCompton thick AGN in the XMM-COSMOS surveySpectral energy distributions of type 1 active galactic nuclei in the COSMOS survey. I. The XMM-COSMOS sampleBolometric luminosities and Eddington ratios of X-ray selected active galactic nuclei in theXMM-COSMOS surveyThe Chandra COSMOS survey. III. Optical and infrared identification of X-ray point sourcesFe K emission from active galaxies in the COSMOS fieldThe bulk of the black hole growth since z ~ 1 occurs in a secular universe: no Major Merger-AGN connectionHot-dust-poor type 1 active galactic nuclei in the COSMOS surveyA runaway black hole in COSMOS: gravitational wave or slingshot recoil?Galaxy-wide outflows inz~ 1.5 luminous obscured quasars revealed through near-IR slit-resolved spectroscopyX-shooter reveals powerful outflows in z ∼ 1.5 X-ray selected obscured quasi-stellar objectsThe mean star-forming properties of QSO host galaxiesEvidence for feedback in action from the molecular gas content in thez~ 1.6 outflowing QSO XID2028Active galactic nucleus X-ray variability in the XMM-COSMOS surveyType 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven QuenchingThe first ultraviolet quasar-stacked spectrum at z ≃ 2.4 from WFC3Is there any evidence that ionized outflows quench star formation in type 1 quasars atz< 1?
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description
Italiaans onderzoeker
@nl
forsker
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researcher ORCID ID = 0000-0003-0083-1157
@en
name
E. Lusso
@ast
E. Lusso
@nl
E. Lusso
@sl
Elisabeta Lusso
@en
Elisabeta Lusso
@es
Elisabeta Lusso
@nb
Elisabeta Lusso
@sq
type
label
E. Lusso
@ast
E. Lusso
@nl
E. Lusso
@sl
Elisabeta Lusso
@en
Elisabeta Lusso
@es
Elisabeta Lusso
@nb
Elisabeta Lusso
@sq
altLabel
E. Lusso
@en
prefLabel
E. Lusso
@ast
E. Lusso
@nl
E. Lusso
@sl
Elisabeta Lusso
@en
Elisabeta Lusso
@es
Elisabeta Lusso
@nb
Elisabeta Lusso
@sq
P106
P1153
35269637500
P27
P31
P496
0000-0003-0083-1157