About: Cristian Vignali

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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 = 0000-0002-8853-9611

Attributes	Values
rdf:type	Item
description	forskare (sv) ikertzailea (eu) 연구원 (ko) 研究者 (ja) araştırmacı (tr) باحت (ary) изилдөөчү (ky) 研究者 (zh) onderzoeker (nl) researcher ORCID ID = 0000-0002-8853-9611 (en)
rdfs:label	Cristian Vignali (en) Cristian Vignali (es) Cristian Vignali (it) Cristian Vignali (nl) Cristian Vignali (ast)
skos:prefLabel	Cristian Vignali (en) Cristian Vignali (es) Cristian Vignali (it) Cristian Vignali (nl) Cristian Vignali (ast)
name	Cristian Vignali (en) Cristian Vignali (es) Cristian Vignali (it) Cristian Vignali (nl) Cristian Vignali (ast)
given name	wds:q58914523-41bd63f8-4e44-c0f1-b39f-1c64b53de118
given name	Cristian
instance of	wds:Q58914523-A4684EA2-D54C-46D6-9094-CF39C3D97E0E
instance of	Homo sapiens
AstroGen ID	wds:Q58914523-4AC111F5-1004-45B2-B1BD-77E673A4428C
AstroGen ID	59365
occupation	wds:Q58914523-B0165529-A22E-44D7-AF27-95A7FE405A5C
sex or gender	wds:Q58914523-AC0B0E7F-6655-4305-A82E-A9DB6236DE20
member of	wds:Q58914523-C268B5D7-F8E7-4079-8DC0-9A20BA924F6B
family name	wds:Q58914523-0C27E084-FBD9-4BAD-91B2-E4948E4E7663
occupation	researcher
sex or gender	male
member of	International Astronomical Union
family name	Vignali
ORCID iD	wds:Q58914523-49135734-9A12-4567-98A6-D6763C8D6BC4
ORCID iD	https://orcid.org/0000-0002-8853-9611
ORCID iD	0000-0002-8853-9611
IRIS UNIBO author ID	wds:Q58914523-FEA3FB41-BE60-4CA3-A2AE-7698A87AF88D
IRIS UNIBO author ID	05130
ResearcherID	wds:Q58914523-B556AA1C-55E5-46BC-9229-2E55ADE81D90
ResearcherID	J-4974-2012
IAU member ID	wds:Q58914523-76607621-06D2-4C97-B6F5-86920D0EE908
IAU member ID	10780
IRIS UNIROMA3 author ID	wds:Q58914523-4292B251-2BC9-438D-8805-70F86A3E4EA5
IRIS UNIROMA3 author ID	47356
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q58914523
is author of	Tracking down the source population responsible for the unresolved cosmic 6-8 keV background The HELLAS2XMM survey Discovery of Compton-thick quasars in the Sloan Digital Sky Survey Molecular gas content in obscured AGN at z > 1 A runaway black hole in COSMOS: gravitational wave or slingshot recoil? The nature of the unresolved extragalactic cosmic soft X-ray background The BeppoSAX High Energy Large Area Survey (HELLAS) -- II. Number counts and X-ray spectral properties TheChandraDeep Field–South Survey: 2 Ms Source Catalogs GOODS-Herschel: ultra-deep XMM-Newton observations reveal AGN/star-formation connection Accreting supermassive black holes in the COSMOS field and the connection to their host galaxies The Chandra COSMOS survey. I. Overview and point source catalog The Chandra Deep Field-South survey: 7 Ms source catalogs The Chandra Deep Field-South survey: 4 Ms source catalogs On the cosmic evolution of the scaling relations between black holes and their host galaxies: broad-line active galactic nuclei in the zCOSMOS survey Compton thick AGN in the XMM-COSMOS survey The population of high-redshift active galactic nuclei in the Chandra-COSMOS survey Identifications and photometric redshifts of the 2 Ms Chandra Deep Field-South sources The XMM-Newton wide-field survey in the COSMOS field. The point-like X-ray source catalogue Chasing highly obscured QSOs in the COSMOS field The most obscured AGN in the COSMOS field X-shooter reveals powerful outflows in z ∼ 1.5 X-ray selected obscured quasi-stellar objects Tracing the cosmic growth of supermassive black holes to z ∼ 3 with Herschel Active galactic nucleus X-ray variability in the XMM-COSMOS survey The hard X-ray luminosity function of high-redshift (3 < z ≲ 5) active galactic nuclei The Complex X‐Ray Absorbers of NGC 3516 Observed byBEPPOSAX High-redshift quasars in the COSMOS survey: the space density of z > 3 X-ray selected QSOs The MBH-M* relation for X-ray-obscured, red QSOs at 1.2 < z < 2.6 The X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOS Galaxy Evolution Studies with the SPace IR Telescope for Cosmology and Astrophysics (SPICA): The Power of IR Spectroscopy NuSTAR REVEALS EXTREME ABSORPTION IN z < 0.5 TYPE 2 QUASARS Detailed shape and evolutionary behavior of the X-ray luminosity function of active galactic nuclei Bolometric luminosities and Eddington ratios of X-ray selected active galactic nuclei in theXMM-COSMOS survey Hot-dust-poor type 1 active galactic nuclei in the COSMOS survey Black hole accretion preferentially occurs in gas-rich galaxies* Obscured AGN at z ~ 1 from the zCOSMOS-Bright Survey The XMM-Newton wide-field survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous active galactic nuclei The Chandra COSMOS survey. III. Optical and infrared identification of X-ray point sources The Chandra-COSMOS survey – IV. X-ray spectra of the bright sample The X-ray to [Ne V]3426 flux ratio: discovering heavily obscured AGN in the distant Universe Unveiling Obscured Accretion in the Chandra Deep Field–South On the nature of red galaxies: the Chandra perspective Resolving the mid-infrared cores of local Seyferts The HELLAS2XMM Survey. I. The X‐Ray Data and the log N–log SRelation Spectroscopic identification of ten faint hard X-ray sources discovered by Chandra On the nature of the X-ray absorption in the Seyfert 2 galaxy NGC 4507 Revealing X-ray obscured quasars in SWIRE sources with extreme mid-IR/optical flux ratios The environments of active galactic nuclei within the zCOSMOS density field A 52 hours VLT/FORS2 spectrum of a bright z ~ 7 HUDF galaxy: no Ly-α emission

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