About: Gian Luigi Granato

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An Entity of Type : wikibase:Item, within Data Space : wikidata.demo.openlinksw.com associated with source document(s)

researcher ORCID ID = 0000-0002-4480-6909

Attributes	Values
rdf:type	Item
description	研究者 (ja) изилдөөчү (ky) onderzoeker (nl) İtalyan araştırmacı (tr) researcher ORCID ID = 0000-0002-4480-6909 (en)
rdfs:label	Gian Luigi Granato (en) Gian Luigi Granato (es) Gian Luigi Granato (it) Gian Luigi Granato (nl) Gian Luigi Granato (sl) Gian Luigi Granato (ast)
skos:prefLabel	Gian Luigi Granato (en) Gian Luigi Granato (es) Gian Luigi Granato (it) Gian Luigi Granato (nl) Gian Luigi Granato (sl) Gian Luigi Granato (ast)
name	Gian Luigi Granato (en) Gian Luigi Granato (es) Gian Luigi Granato (it) Gian Luigi Granato (nl) Gian Luigi Granato (sl) Gian Luigi Granato (ast)
given name	wds:Q58916569-8F44B9BD-A6A7-4134-A6EF-998C291E47B0
given name	Gian
instance of	wds:Q58916569-B2AE4E61-3060-454F-8BE9-7E091801E84E
instance of	Homo sapiens
work location	wds:Q58916569-A0A78109-3D2F-447E-8FD0-8827287540C4
work location	Padua
occupation	wds:Q58916569-7A35505E-B811-4605-BDC7-E3C4561EABD7
employer	wds:Q58916569-7651a826-4485-572e-1441-bcb9bf1a0140
sex or gender	wds:Q58916569-DEDD543C-06ED-4933-B7FA-144F6ADA6ADA
country of citizenship	wds:Q58916569-36e9f9e5-4fb1-ba0b-a685-90881446e70b
member of	wds:Q58916569-FFEC1F22-C8C0-4BBD-8872-C0801B059B1B
family name	wds:Q58916569-8ad823ad-42fe-e357-ab7b-9838acb1c647
occupation	researcher
employer	Astronomical Observatory of Padova
sex or gender	male
country of citizenship	Italy
member of	International Astronomical Union
family name	Granato
Springer Nature person ID	wds:Q58916569-56967226-1267-4740-9535-AC28669DCF48
ORCID iD	wds:Q58916569-98D399E3-9B37-4856-804B-4DDDD8576BB9
Dimensions author ID	wds:Q58916569-758EB535-5253-4190-9650-7F7AB4C512CC
ORCID iD	https://orcid.org/0000-0002-4480-6909
Springer Nature person ID	016303446335.27
ORCID iD	0000-0002-4480-6909
Dimensions author ID	016303446335.27
ArTS author ID	wds:Q58916569-81D7F093-F01D-445F-A50E-8F25E7E200AB
ArTS author ID	12483
IAU member ID	wds:Q58916569-9678D759-CEFE-4F28-8495-FE4B6E853873
IAU member ID	10764
SISSA Digital Library author ID	wds:Q58916569-45E17559-CD6B-45D7-A151-2AE55C7B5E8C
SISSA Digital Library author ID	00283
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q58916569
is author of	AMAZE. I. The evolution of the mass-metallicity relation at z>3 Evolution of asymptotic giant branch stars. II. Optical to far-infrared isochrones with improved TP-AGB models The SCUBA Half-Degree Extragalactic Survey - II. Submillimetre maps, catalogue and number counts The SCUBA Half-Degree Extragalactic Survey -- I. Survey motivation, design and data processing Predictions for the SKA from hierarchical galaxy formation models Comparison of star formation rates from Hα and infrared luminosity as seen byHerschel Modelling the effects of dust evolution on the SEDs of galaxies of different morphological type The dust content of high-z submillimeter galaxies revealed by Herschel Can the faint submillimetre galaxies be explained in the Λ cold dark matter model? The Infrared Side of Galaxy Formation. I. The Local Universe in the Semianalytical Framework Galaxy evolution in the infrared: comparison of a hierarchical galaxy formation model with Spitzer data Infrared space observatory investigates the nature of extremely red hard X-ray sources responsible for the X-ray background The role of the synchrotron component in the mid-infrared spectrum of M 87 Black hole accretion preferentially occurs in gas-rich galaxies* Dust and nebular emission. I. Models for normal galaxies Thick tori around active galactic nuclei: a comparison of model predictions with observations of the infrared continuum and silicate features A physical model for the coevolution of QSOs and their spheroidal hosts Joint formation of QSOs and spheroids: QSOs as clocks of star formation in spheroids Modeling the effects of dust on galactic spectral energy distributions from the ultraviolet to the millimeter band Chemical abundances in QSO host galaxies and environments from narrow absorption line systems Connecting the cosmic infrared background to the X-ray background Predictions forHerschelfrom Λ-cold dark matter: unveiling the cosmic star formation history Two-phase galaxy formation: the evolutionary properties of galaxies The European Large-Area ISO Survey (ELAIS): the final band-merged catalogue Observations of the Hubble Deep Field South with the Infrared Space Observatory- I. Observations, data reduction and mid-infrared source counts Observations of the Hubble Deep Field South with the Infrared Space Observatory- II. Associations and star formation rates The European Large Area ISO Survey -- I. Goals, definition and observations Thick tori around active galactic nuclei: the case for extended tori and consequences for their X-ray and infrared emission The role of the dust in primeval galaxies: a simple physical model for Lyman break galaxies and Ly{alpha} emitters Dust-enshrouded AGN models for hyperluminous, high-redshift infrared galaxies Exploring supermassive black hole growth with ALMA The SCUBA HAlf Degree Extragalactic Survey (SHADES) - V. Submillimetre properties of near-infrared-selected galaxies in the Subaru/XMM-Newton deep field The evolution of actively star-forming galaxies in the mid-infrared NGC 3741: the dark halo profile from the most extended rotation curve Cool core clusters from cosmological simulations Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution Halo cluster shapes: insights from simulated galaxies and ICL with prospects for weak lensing applications wd:Q58910268 Early-type galaxies in the Hubble Deep Field: the star formation history New photometric models of galactic evolution applied to the HDF Are the bulk of z > 2 Herschel galaxies proto-spheroids? Far infrared and radio emission in dusty starburst galaxies The mid-infrared colour-magnitude relation of early-type galaxies in the Coma cluster as measured by Spitzer-IRS A study of a homogeneous sample of optically selected active galactic nuclei. III. Optical observations

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