about
Cosmic CARNage II: the evolution of the galaxy stellar mass functionin observations and galaxy formation modelsnIFTy cosmology: the clustering consistency of galaxy formation modelsnIFTy cosmology: comparison of galaxy formation modelsThe Space Density of High-Redshift QSOs in the Great Observatories Origins Deep SurveyOn the evolution of the cosmic ionizing backgroundOn the relative contribution of high-redshift galaxies and active galactic nuclei to reionizationOn the evolution of the star formation rate function of massive galaxies: constraints at from the GOODS-MUSIC catalogueThe great observatories origins deep survey: constraints on the Lyman continuum escape fraction distribution of lyman-break galaxies at 3.4 < z < 4.5Faint Lyman-break galaxies as a crucial test for galaxy formation modelsStar formation and mass assembly in high redshift galaxiesThe quasar proximity effect at redshift 〈z〉≃ 2.6 with the From Lines to Overdensities approach★The luminosity function of high-redshift quasi-stellar objects. A combined analysis of GOODS and SDSSBlack Hole Masses and Eddington Ratios of AGNs atz< 1: Evidence of Retriggering for a Representative Sample of X‐Ray‐selected AGNsThe Galaxy mass function up to z $\mathsf{=4}$ in the GOODS-MUSIC sample: into the epoch of formation of massive galaxiesThe effect of stellar feedback and quasar winds on the active galactic nucleus populationThe evolving slope of the stellar mass function at 0.6 ≤ z< 4.5 from deep WFC3 dataWide and deep near-UV (360 nm) galaxy counts and the extragalactic background light with the Large Binocular CameraObservational constraints on the co-evolution of supermassive black holes and galaxiesSemi-analytic galaxy formation in coupled dark energy cosmologiesSemi-analytic galaxy formation in f(R)-gravity cosmologiesSemi-analytic galaxy formation in early dark energy cosmologiesStar formation inHerschel's Monsters versus semi-analytic modelsThe correlation of star formation quenching with internal galaxy properties and environmentA semi-analytic model comparison: testing cooling models against hydrodynamical simulationsA semi-analytic model comparison - gas cooling and galaxy mergersThe effect of thermally pulsating asymptotic giant branch stars on the evolution of the rest-frame near-infrared galaxy luminosity functionThe many manifestations of downsizing: hierarchical galaxy formation models confront observationsMetals in thez∼ 3 intergalactic medium: results from an ultra-high signal-to-noise ratio UVES quasar spectrum
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description
researcher, ORCID id # 0000-0003-4744-0188
@en
wetenschapper
@nl
name
Fabio Fontanot
@ast
Fabio Fontanot
@en
Fabio Fontanot
@es
Fabio Fontanot
@nl
type
label
Fabio Fontanot
@ast
Fabio Fontanot
@en
Fabio Fontanot
@es
Fabio Fontanot
@nl
prefLabel
Fabio Fontanot
@ast
Fabio Fontanot
@en
Fabio Fontanot
@es
Fabio Fontanot
@nl
P106
P21
P31
P496
0000-0003-4744-0188