about
Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10¹¹ solar massesHerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurementsA dust-obscured massive maximum-starburst galaxy at a redshift of 6.34.The suppression of star formation by powerful active galactic nucleiA multidimensional version of the Kolmogorov–Smirnov testObservations of the Hubble Deep Field with the Infrared Space Observatory - V. Spectral energy distributions, starburst models and star formation historyHerMES: CANDIDATE GRAVITATIONALLY LENSED GALAXIES AND LENSING STATISTICS AT SUBMILLIMETER WAVELENGTHSTheHerschel-SPIRE instrument and its in-flight performanceHerschel-ATLAS: a binary HyLIRG pinpointing a cluster of starbursting protoellipticalsThe Spitzer Extragalactic Representative Volume Survey (SERVS): Survey Definition and Goals*The Spitzer Extragalactic Representative Volume Survey (SERVS): Survey Definition and Goals ( PASP, 124, 714, [2012] )Herscheland SCUBA-2 imaging and spectroscopy of a bright, lensed submillimetre galaxy atz= 2.3SPACE: the spectroscopic all-sky cosmic explorerCOSMOS: Hubble Space Telescope ObservationsCold dust and young starbursts: spectral energy distributions of Herschel SPIRE sources from the HerMES survey★Evolution of dust temperature of galaxies through cosmic time as seen by HerschelFirst results from HerMES on the evolution of the submillimetre luminosity functionHerMES: deep galaxy number counts from a P(D) fluctuation analysis of SPIRE Science Demonstration Phase observationsHerMES: Far infrared properties of known AGN in the HerMES fieldsHerMES: The SPIRE confusion limitHerMES: The submillimeter spectral energy distributions of Herschel/SPIRE-detected galaxiesHerschel unveils a puzzling uniformity of distant dusty galaxiesMeasures of star formation rates from infrared (Herschel) and UV (GALEX) emissions of galaxies in the HerMES fieldsThe Deep SPIRE HerMES Survey: spectral energy distributions and their astrophysical indications at high redshiftThe HerMES SPIRE submillimeter local luminosity functionThe Herschel Multi-Tiered Extragalactic Survey: source extraction and cross-identifications in confusion-dominated SPIRE imagesThe far-infrared/radio correlation as probed by HerschelRemarkable Disk and Off-Nuclear Starburst Activity in the Tadpole Galaxy as revealed by theSpitzer Space TelescopeHerMES: LYMAN BREAK GALAXIES INDIVIDUALLY DETECTED AT 0.7 ⩽ z ⩽ 2.0 IN GOODS-N WITH HERSCHEL/SPIREThe European Large-Area ISO Survey (ELAIS): the final band-merged catalogueObservations of the Hubble Deep Field South with the Infrared Space Observatory- I. Observations, data reduction and mid-infrared source countsObservations of the Hubble Deep Field South with the Infrared Space Observatory- II. Associations and star formation ratesThe European Large Area ISO Survey -- I. Goals, definition and observationsObservations of the Hubble Deep Field with the Infrared Space Observatory - I. Data reduction, maps and sky coverageObservations of the Hubble Deep Field with the Infrared Space Observatory - II. Source detection and photometryObservations of the Hubble Deep Field with the Infrared Space Observatory - III. Source counts and P(D) analysisObservations of the Hubble Deep Field with the Infrared Space Observatory - IV. Association of sources with Hubble Deep Field galaxiesQuasars Classes and Their RelationshipsThe Future of Quasar StudiesDynamical masses of early-type galaxies at z ~ 2: are they truly superdense?
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description
Itaalia astronoom
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Italiaans astronoom
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Italian astronomer
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Italian astronomer
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Italian astronomer
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astronom italian
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Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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prefLabel
Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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Alberto Franceschini
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1952-02-17T00:00:00Z