Publication data of Trenti, Michele: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2010202020052015202502000400060008000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications201020202005201520250306090120150048121620
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion20022004200620082010201220142016201820202022202401020304050
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestStar formation rates and stellar masses of z=7-8 galaxies from IRAC observations of the WFC3/IR ERS and the HUDF fieldStar formation rates and stellar masses of z=7-8 galaxies from IRAC observati…The Galaxy Luminosity Function during the Reionization EpochStructure and Morphologies of z~7-8 Galaxies from ultra-deep WFC3/IR Imaging of the HUDFStructure and Morphologies of z~7-8 Galaxies from ultra-deep WFC3/IR Imagi…Probing the Dawn of Galaxies at $z sim$ 9-12: New Constraints from HUDF12/XDF and CANDELS dataProbing the Dawn of Galaxies at $z sim$ 9-12: New Constraints from HUDF12…The Galaxy UV Luminosity Function Before the Epoch of ReionizationThe Most Luminous $z sim$ 9-10 Galaxy Candidates Yet Found: The Luminosity Function, Cosmic Star-formation Rate, and the First Mass Density Estimate at 500 MyrThe Most Luminous $z sim$ 9-10 Galaxy Candidates Yet Found: The Luminosi…Very blue UV-continuum slopes of low luminosity z~7 galaxies from WFC3/IR: Evidence for extremely low metallicities?Very blue UV-continuum slopes of low luminosity z~7 galaxies from WFC3/IR: …Inferences on the timeline of reionization at z ∼ 8 from the KMOS Lens-Amplified Spectroscopic SurveyInferences on the timeline of reionization at z ∼ 8 from the KMOS Lens-Amplif…The Formation Rates of Population III Stars and Chemical Enrichment of Halos during the Reionization EraThe Formation Rates of Population III Stars and Chemical Enrichment of Halo…Lower-Luminosity Galaxies could reionize the Universe: Very Steep Faint-End Slopes to the UV Luminosity Functions at z>=5-8 from the HUDF09 WFC3/IR ObservationsLower-Luminosity Galaxies could reionize the Universe: Very Steep Faint-End …Cosmic Variance and Its Effect on the Luminosity Function Determination in Deep High z SurveysCosmic Variance and Its Effect on the Luminosity Function Determination in …z~7 Galaxies in the HUDF: First Epoch WFC3/IR ResultsUV-Continuum Slopes of >4000 $z sim$ 4-8 Galaxies from the HUDF/XDF, HUDF09, ERS, CANDELS-South, and CANDELS-North FieldsUV-Continuum Slopes of >4000 $z sim$ 4-8 Galaxies from the HUDF/XDF, HU…A candidate redshift z ~ 10 galaxy and rapid changes in that population at an age of 500 MyrA candidate redshift z ~ 10 galaxy and rapid changes in that population at a…The Universe Is Reionizing at z ∼ 7: Bayesian Inference of the IGM Neutral Fraction Using Ly$alpha$ Emission from GalaxiesThe Universe Is Reionizing at z ∼ 7: Bayesian Inference of the IGM Neutral Fra…UV-continuum slopes at z~4-7 from the HUDF09+ERS+CANDELS observations: Discovery of a well-defined UV-color magnitude relationship for z>=4 star-forming galaxiesUV-continuum slopes at z~4-7 from the HUDF09+ERS+CANDELS observatio…Discovery of z~8 Galaxies in the HUDF from ultra-deep WFC3/IR ObservationsUV Luminosity Functions from 113 z~7 and z~8 Lyman-Break Galaxies in the ultra-deep HUDF09 and wide-area ERS WFC3/IR ObservationsUV Luminosity Functions from 113 z~7 and z~8 Lyman-Break Galaxies in the…UV Luminosity Functions at redshifts $z sim$4 to $z sim$10: 10000 Galaxies from HST Legacy FieldsUV Luminosity Functions at redshifts $z sim$4 to $z sim$10: 10000 Galaxies…2010202020052015202502000400060008000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Star formation rates and stellar masses of z=7-8 galaxies from IRAC observations of the WFC3/IR ERS and the HUDF fieldStar formation rates and stellar masses of z=7-8 galaxies from IRAC observati…The Galaxy Luminosity Function during the Reionization EpochStructure and Morphologies of z~7-8 Galaxies from ultra-deep WFC3/IR Imaging of the HUDFStructure and Morphologies of z~7-8 Galaxies from ultra-deep WFC3/IR Imagi…Probing the Dawn of Galaxies at $z sim$ 9-12: New Constraints from HUDF12/XDF and CANDELS dataProbing the Dawn of Galaxies at $z sim$ 9-12: New Constraints from HUDF12…The Galaxy UV Luminosity Function Before the Epoch of ReionizationThe Most Luminous $z sim$ 9-10 Galaxy Candidates Yet Found: The Luminosity Function, Cosmic Star-formation Rate, and the First Mass Density Estimate at 500 MyrThe Most Luminous $z sim$ 9-10 Galaxy Candidates Yet Found: The Luminosi…Very blue UV-continuum slopes of low luminosity z~7 galaxies from WFC3/IR: Evidence for extremely low metallicities?Very blue UV-continuum slopes of low luminosity z~7 galaxies from WFC3/IR: …Inferences on the timeline of reionization at z ∼ 8 from the KMOS Lens-Amplified Spectroscopic SurveyInferences on the timeline of reionization at z ∼ 8 from the KMOS Lens-Amplif…The Formation Rates of Population III Stars and Chemical Enrichment of Halos during the Reionization EraThe Formation Rates of Population III Stars and Chemical Enrichment of Halo…Lower-Luminosity Galaxies could reionize the Universe: Very Steep Faint-End Slopes to the UV Luminosity Functions at z>=5-8 from the HUDF09 WFC3/IR ObservationsLower-Luminosity Galaxies could reionize the Universe: Very Steep Faint-End …Cosmic Variance and Its Effect on the Luminosity Function Determination in Deep High z SurveysCosmic Variance and Its Effect on the Luminosity Function Determination in …z~7 Galaxies in the HUDF: First Epoch WFC3/IR ResultsUV-Continuum Slopes of >4000 $z sim$ 4-8 Galaxies from the HUDF/XDF, HUDF09, ERS, CANDELS-South, and CANDELS-North FieldsUV-Continuum Slopes of >4000 $z sim$ 4-8 Galaxies from the HUDF/XDF, HU…A candidate redshift z ~ 10 galaxy and rapid changes in that population at an age of 500 MyrA candidate redshift z ~ 10 galaxy and rapid changes in that population at a…The Universe Is Reionizing at z ∼ 7: Bayesian Inference of the IGM Neutral Fraction Using Ly$alpha$ Emission from GalaxiesThe Universe Is Reionizing at z ∼ 7: Bayesian Inference of the IGM Neutral Fra…UV-continuum slopes at z~4-7 from the HUDF09+ERS+CANDELS observations: Discovery of a well-defined UV-color magnitude relationship for z>=4 star-forming galaxiesUV-continuum slopes at z~4-7 from the HUDF09+ERS+CANDELS observatio…Discovery of z~8 Galaxies in the HUDF from ultra-deep WFC3/IR ObservationsUV Luminosity Functions from 113 z~7 and z~8 Lyman-Break Galaxies in the ultra-deep HUDF09 and wide-area ERS WFC3/IR ObservationsUV Luminosity Functions from 113 z~7 and z~8 Lyman-Break Galaxies in the…UV Luminosity Functions at redshifts $z sim$4 to $z sim$10: 10000 Galaxies from HST Legacy FieldsUV Luminosity Functions at redshifts $z sim$4 to $z sim$10: 10000 Galaxies…2002200420062008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average2002200420062008201020122014201620182020202220240200400600800