About: The X-ray to [Ne V]3426 flux ratio: discovering heavily obscured AGN in the distant Universe

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About: The X-ray to [Ne V]3426 flux ratio: discovering heavily obscured AGN in the distant Universe Goto Sponge NotDistinct Permalink

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scientific article published in Astronomy and Astrophysics

Attributes	Values
rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) наукова стаття, опублікована у вересні 2010 (uk) im September 2010 veröffentlichter wissenschaftlicher Artikel (de) article publié dans la revue scientifique Astronomy and Astrophysics (fr) scientific article published in Astronomy and Astrophysics (en)
publication date	wds:Q58910736-47DABB47-D730-46C3-AF06-71ED11173F6A
publication date	2010-09-01 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q58910736-D275FDD9-900F-4492-9E1F-AEB6E5AD3A59
language of work or name	English
cites work	wds:Q58910736-AC0A20FA-90EA-48CD-AD11-49399136EEBC
cites work	Spectrophotometry of active galaxies - I. The observations
author name string	wds:Q58910736-B51660A2-146A-4FB2-88C3-B99F10B98B19
author name string	R. Gilli
rdfs:label	The X-ray to [Ne V]3426 flux ratio: discovering heavily obscured AGN in the distant Universe (en) The X-ray to [Ne V]3426 flux ratio: discovering heavily obscured AGN in the distant Universe (nl)
skos:prefLabel	The X-ray to [Ne V]3426 flux ratio: discovering heavily obscured AGN in the distant Universe (en) The X-ray to [Ne V]3426 flux ratio: discovering heavily obscured AGN in the distant Universe (nl)
name	The X-ray to [Ne V]3426 flux ratio: discovering heavily obscured AGN in the distant Universe (en) The X-ray to [Ne V]3426 flux ratio: discovering heavily obscured AGN in the distant Universe (nl)
author	wds:Q58910736-783DD899-A71D-4F50-B58A-2C31C1C111DF wds:Q58910736-96C23549-7E97-4D52-935C-2D828B4B509E wds:Q58910736-B0B6EE12-BFAB-4AB2-BD85-02C169129352 wds:Q58910736-B82B239E-4E78-41BD-B064-2E94DB310FA4 wds:Q58910736-DA5B8A3B-B1AF-4BD3-90C2-5E3815014ECE
author	Andrea Comastri Marco Mignoli Giovanni Zamorani Kazushi Iwasawa Cristian Vignali
title	wds:Q58910736-8EA576FB-9D3C-44CB-AA10-EBA14BAB814B
title	The X-ray to [Ne V]3426 flux ratio: discovering heavily obscured AGN in the distant Universe (en)
page(s)	wds:Q58910736-C7B4452F-7A12-4C18-AC52-BFA3B29B3F5C
page(s)	92–92
instance of	wds:Q58910736-4640BCD3-1B34-4BA9-85BD-3B41A5F2B4F4
instance of	scholarly article
published in	wds:Q58910736-7DA86990-5CCF-475B-8284-58905B83F2F3
published in	Astronomy and Astrophysics
volume	wds:Q58910736-FDD7A556-4930-417E-B094-217D13FB167F
volume	519
DOI	wds:Q58910736-0636A3C6-471B-4670-AD54-3D81CD82C2D1
DOI	http://dx.doi.org/10.1051/0004-6361/201014039
DOI	10.1051/0004-6361/201014039
Fatcat ID	wds:Q58910736-F6DF90A1-5562-4975-B13A-A8BEA3AECFF6
Fatcat ID	release_7oqottgrfbcvfdqj2eumnkomtq
arXiv ID	wds:Q58910736-BFE26F7B-9AFB-4BA7-9B67-FABC74D60819
arXiv ID	1005.0373
ADS bibcode	wds:Q58910736-787CD557-858D-49E9-A039-7DC7CEB28186
ADS bibcode	2010A&A...519A..92G
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q58910736
is cites work of	Accreting supermassive black holes in the COSMOS field and the connection to their host galaxies The most obscured AGN in the COSMOS field Tracing the cosmic growth of supermassive black holes to z ∼ 3 with Herschel Massive compact galaxies with high-velocity outflows: morphological analysis and constraints on AGN activity Exploring the active galactic nuclei population with extreme X-ray-to-optical flux ratios (fx/fo > 50) Obscured AGN at z ~ 1 from the zCOSMOS-Bright Survey The XMM deep survey in the CDF-S. IV. Compton-thick AGN candidates On theLx–L6 μmratio as a diagnostic for Compton-thick AGN A wide search for obscured active galactic nuclei using XMM–Newton and WISE TheXMMDeep survey in the CDF-S Black hole accretion and host galaxies of obscured quasars in XMM-COSMOS The incidence of obscuration in active galactic nuclei AGN host galaxy mass function in COSMOS The space density of Compton-thick AGN atz≈ 0.8 in the zCOSMOS-Bright Survey A 100-kiloparsec wind feeding the circumgalactic medium of a massive compact galaxy San Pedro Mártir observations of microvariability in obscured quasars
is cites work of	wds:Q57676234-5BEE5328-4B05-4C6D-B00E-90907582D355 wds:Q58910687-C686DE0A-FC3B-44F3-B25C-A80520FA8644 wds:Q58912181-D34B785A-1CCD-4A06-B104-7F5C4F8945B8 wds:Q58912217-5B4F309D-E632-426B-A8C3-34F13AC1B255 wds:Q58786228-B623C74E-F790-4F16-B271-E5A6D304828C wds:Q58035465-69458A8D-076A-48FB-A848-5ECC886E44D2 wds:Q58910622-8C6E659A-1C36-4203-B8AB-86C97FF5F0F5 wds:Q58909598-2BD2167D-C014-4F53-9448-9E22BA15676D wds:Q58910684-618F71D8-B754-4439-9FCC-0BD21723544B wds:Q58912204-7D0461C2-17E3-4AB1-B830-CFDBA3B03D74 wds:Q57686628-E6D14CCB-FD23-4421-882D-2286AD15D7C9 wds:Q58921815-1A57FCDD-5C37-44A6-ACA6-55C8F47111EB wds:Q58035559-8F56B838-B546-4382-AC59-528DB187B56D wds:Q58910662-7599EC7C-6511-4987-A376-FEF21EFDB7F6 wds:Q91013894-CEE52F11-27FE-4E8F-9DD5-3CF6A08A7F80 wds:Q56924468-207AC4A1-AE8F-4B8B-BA7B-F7CBA92BA373

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