About: Roberto Gilli

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

Italian astrophysicist (1973-)

Attributes	Values
rdf:type	Item
description	wetenschapper (nl) дослідник (uk) Italian astrophysicist (1973-) (en) astrofisico italiano (1973-) (it)
exact match	wds:Q58920927-397D3F06-A46D-4359-B45C-A4C80C41F4E9
exact match	https://scigraph.springernature.com/person.013323313243.06
rdfs:label	Roberto Gilli (de) Roberto Gilli (en) Roberto Gilli (es) Roberto Gilli (fr) Roberto Gilli (it) Roberto Gilli (nl) Roberto Gilli (pt) Roberto Gilli (sl) Roberto Gilli (pt-br) Roberto Gilli (ast)
skos:prefLabel	Roberto Gilli (de) Roberto Gilli (en) Roberto Gilli (es) Roberto Gilli (fr) Roberto Gilli (it) Roberto Gilli (nl) Roberto Gilli (pt) Roberto Gilli (sl) Roberto Gilli (pt-br) Roberto Gilli (ast)
name	Roberto Gilli (de) Roberto Gilli (en) Roberto Gilli (es) Roberto Gilli (fr) Roberto Gilli (it) Roberto Gilli (nl) Roberto Gilli (pt) Roberto Gilli (sl) Roberto Gilli (pt-br) Roberto Gilli (ast)
Scopus author ID	wds:Q58920927-0483ED31-7C4F-489E-A7A3-093C36AAEC5E
Scopus author ID	56253699200
given name	wds:Q58920927-313C5D86-D03C-4C3D-8744-7752703FF54E
given name	Roberto
instance of	wds:Q58920927-34D274B5-8230-4DF0-BD49-C0F0866663E8
instance of	Homo sapiens
curriculum vitae URL	wds:Q58920927-ad1f0488-4ed3-e565-2a9e-6b61c4eb83b4
IRIS SNS author ID	wds:Q58920927-2E1ECBDD-7568-4D02-ACF9-D20F6AC8D6C6
curriculum vitae URL	http://www.bo.astro.it/wp-content/uploads/2017/12/CV-gilli.pdf
IRIS SNS author ID	30226
occupation	wds:Q58920927-5C6484FF-097A-45B8-BDE6-18D2E3ADA5DC
languages spoken, written or signed	wds:q58920927-c2ee4860-41fe-fc18-22e7-2bc9e1fd51bd wds:q58920927-fd3e1bba-41f0-5c9e-1f78-5c375e6a2903
place of birth	wds:q58920927-319cb23c-47e0-3cfa-02ff-8505bc27bc0d
sex or gender	wds:Q58920927-8f4ccc96-4298-3e92-12fe-5d7246e0b629
country of citizenship	wds:q58920927-2437a2f1-429b-84ec-c2af-1be5630df737
date of birth	wds:Q58920927-4effae48-4a0c-8b54-82e4-3cff0577a4fb
educated at	wds:Q58920927-18C245E8-1E20-4BAB-8C90-656F40CFE318
family name	wds:Q58920927-5DDCC910-94A6-456E-8AF9-3A46DBFD7190
occupation	astrophysicist
languages spoken, written or signed	English Italian
place of birth	Ferrara
sex or gender	male
country of citizenship	Italy
date of birth	1973-01-25 00:00:00Z (xsd:dateTime)
educated at	National Institute for Astrophysics
family name	Gilli
ORCID iD	wds:Q58920927-E6FA7394-58D1-4D51-80BE-84D230CB30EE
Dimensions author ID	wds:Q58920927-075CE5ED-54B6-4E51-B08E-DDFD282878AB
ORCID iD	https://orcid.org/0000-0001-8121-6177
ORCID iD	0000-0001-8121-6177
Dimensions author ID	013323313243.06
FLORE author ID	wds:Q58920927-1CD515E0-D086-4704-91B0-0ABC46C2E2BC
FLORE author ID	38357
ResearcherID	wds:Q58920927-B664528F-2CB5-47DB-AB5B-2B8AE25F5BDE
ResearcherID	P-1110-2015
is owl:sameAs of	Roberto Gilli
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q58920927
is author of	The Chandra COSMOS survey. I. Overview and point source catalog ChandraDeep Field South: The 1 Ms Catalog A Classic Type 2 QSO RADIO LOUD AGNs ARE MERGERS The X‐Ray–derived Cosmological Star Formation History and the Galaxy X‐Ray Luminosity Functions in the Chandra Deep Fields North and South Unresolved z ∼ 8 Point Sources and Their Impact on the Bright End of the Galaxy Luminosity Function X-UDS: The Chandra Legacy Survey of the UKIDSS Ultra Deep Survey Field Rolling down from the 30 keV peak: Modelling the hard X-ray and γ-ray backgrounds Rolling down from the 30 keV peak: Modelling the Hard X-Ray and γ-Ray Backgrounds Erratum: “X-Ray Properties of AGN in Brightest Cluster Galaxies. I. A Systematic Study of the <i>Chandra</i> Archive in the 0.2 < <i>z</i> < 0.3 and 0.55 < <i>z</i> < 0.75 Redshift Range” (2018, ApJ, 859, 65) The evolution of obscured accretion The Iron Line Background The cosmic reality check EXTraS discovery of an X-ray superflare from an L dwarf Supermassive black holes at high redshift are expected to be obscured by their massive host galaxies’ interstellar medium XEUS: the physics of the hot evolving universe Discovery of a galaxy overdensity around a powerful, heavily obscured FRII radio galaxy at<i>z</i>= 1.7: star formation promoted by large-scale AGN feedback? TheXMM‐NewtonWide‐Field Survey in the COSMOS Field. V. Angular Clustering of the X‐Ray Point Sources The spatial distribution of X-ray selected AGN in theChandradeep fields: a theoretical perspective X-Ray Spectral Analyses of AGNs from the 7Ms Chandra Deep Field-South Survey: The Distribution, Variability, and Evolutions of AGN Obscuration
is author of	wds:Q58909113-C072E4EC-5B8C-40FD-B790-0B233947B308 wds:Q114022989-DC6BAAA3-ACED-452F-A67F-CE07F41CE8AF wds:Q59715942-0DD3E8A0-74C6-4E34-A5B5-8DC1C1018905 wds:Q58912293-049E09D6-948F-4AD7-9B6B-E22FC42B0414

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