Publication data of Stiavelli, Massimo: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion199520002005201020152020202502000400060008000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1995200020052010201520202025025507510012503691215
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion199520002005201020152020202501020304050
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe properties of field elliptical galaxies at intermediate redshift. 2. photometry and spectroscopy of an hst selected sampleThe properties of field elliptical galaxies at intermediate redshift. 2. photomet…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 properties of field elliptical galaxies at intermediate redshift. I: empirical scaling lawsThe properties of field elliptical galaxies at intermediate redshift. I: empirical …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…The evolution of field early-type galaxies to Z 0.7Probing 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…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: …WFPC2 Observations of the Hubble Deep Field SouthSpiral galaxies with wfpc2. 2. The nuclear properties of 40 objectsThe 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 ResultsA 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…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…The Hubble Ultra Deep FieldPassively evolving early-type galaxies at 1.4 <~ z <~ 2.5 in the Hubble Ultra Deep FieldPassively evolving early-type galaxies at 1.4 <~ z <~ 2.5 in the Hubble Ultra …199520002005201020152020202502000400060008000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The properties of field elliptical galaxies at intermediate redshift. 2. photometry and spectroscopy of an hst selected sampleThe properties of field elliptical galaxies at intermediate redshift. 2. photomet…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 properties of field elliptical galaxies at intermediate redshift. I: empirical scaling lawsThe properties of field elliptical galaxies at intermediate redshift. I: empirical …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…The evolution of field early-type galaxies to Z 0.7Probing 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…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: …WFPC2 Observations of the Hubble Deep Field SouthSpiral galaxies with wfpc2. 2. The nuclear properties of 40 objectsThe 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 ResultsA 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…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…The Hubble Ultra Deep FieldPassively evolving early-type galaxies at 1.4 <~ z <~ 2.5 in the Hubble Ultra Deep FieldPassively evolving early-type galaxies at 1.4 <~ z <~ 2.5 in the Hubble Ultra …19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19952000200520102015202020250200400600800