About: HerMES: current cosmic infrared background estimates can Be explained by known galaxies and their faint companions at z

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About: HerMES: current cosmic infrared background estimates can Be explained by known galaxies and their faint companions at z < 4 Goto Sponge NotDistinct Permalink

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rdf:type	Item
description	article (en) wetenschappelijk artikel (nl) наукова стаття, опублікована в серпні 2015 (uk) im August 2015 veröffentlichter wissenschaftlicher Artikel (de)
publication date	wds:Q58217077-0C84E2B4-C62A-47AE-BE2E-6E59425F0885
publication date	2015-08-18 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q58217077-F6BCB92E-A157-479C-BD85-56913F91ABD6
language of work or name	English
author name string	wds:Q58217077-0E43BBFE-B68C-439E-B56C-48BF39024414 wds:Q58217077-21EC3CC0-7929-42F2-B476-967FDC13637F wds:Q58217077-3A836C48-BC4D-4AC2-93CA-A5CD3432D521 wds:Q58217077-3B951E90-975C-4B42-A5F7-67DC8B5D0C74 wds:Q58217077-3BDECEF1-4191-4A39-B6BB-63AEDB5714D4 wds:Q58217077-42E77ED0-17F9-4C8F-9291-620F5BCC5DE6 wds:Q58217077-5904ED90-23F9-4200-A2CB-A6FFAFD5E717 wds:Q58217077-8537072C-7210-4A62-B8D9-D0534797AA85 wds:Q58217077-982D2E83-2A51-4A0F-B734-D73B631DA449 wds:Q58217077-A6B12248-3766-43EF-A390-B05B3812EB01 wds:Q58217077-BBAF6BB5-BFFA-4A42-B53D-7584F2EA1182 wds:Q58217077-C4CF15A0-557C-4A4F-B3AD-BC0FC04667CA wds:Q58217077-DC0769A0-F983-41F9-9C49-4155615C2FA6 wds:Q58217077-F25D2B06-3313-4F15-A297-691FAF481D04 wds:Q58217077-FD3D848F-A5BE-4D16-8ECC-0421D7674CF1 wds:Q58217077-FE25CA64-2F1D-4714-B5A5-DB45D180326E
author name string	L. Wang B. Schulz M. Halpern M. J. Page J. Bock D. L. Clements G. Marsden A. Conley I. Valtchanov M. Zemcov S. C. Chapman S. J. Oliver I. Pérez-Fournon M. P. Viero R. F. Quadri S. Duivenvoorden
rdfs:label	HerMES: current cosmic infrared background estimates can Be explained by known galaxies and their faint companions at z < 4 (en) HERMES: CURRENT COSMIC INFRARED BACKGROUND ESTIMATES CAN BE EXPLAINED BY KNOWN GALAXIES AND THEIR FAINT COMPANIONS AT z < 4 (nl)
skos:prefLabel	HerMES: current cosmic infrared background estimates can Be explained by known galaxies and their faint companions at z < 4 (en) HERMES: CURRENT COSMIC INFRARED BACKGROUND ESTIMATES CAN BE EXPLAINED BY KNOWN GALAXIES AND THEIR FAINT COMPANIONS AT z < 4 (nl)
name	HerMES: current cosmic infrared background estimates can Be explained by known galaxies and their faint companions at z < 4 (en) HERMES: CURRENT COSMIC INFRARED BACKGROUND ESTIMATES CAN BE EXPLAINED BY KNOWN GALAXIES AND THEIR FAINT COMPANIONS AT z < 4 (nl)
author	wds:Q58217077-04BBC5A3-266B-4BDF-A5D8-69523A42B04F wds:Q58217077-1C832579-4D0E-420C-A699-39349461BFAC wds:Q58217077-2FC7BC82-C429-414D-AA20-F39E51FFEC49 wds:Q58217077-43361341-2D8B-4224-91EC-D32B8C6740AE wds:Q58217077-47C23D26-D692-4620-AB50-24318668BAFC wds:Q58217077-606325FA-6EA4-463A-B9CE-6AAFD2C5FE18 wds:Q58217077-68F4C892-76BA-4764-B84E-AC9BC64776E9 wds:Q58217077-6CB5B668-E046-463A-8A71-E47A256A06D2 wds:Q58217077-7BE3A813-4063-4005-8058-39C9622705BA wds:Q58217077-9AFCC981-4769-4EAB-AEF0-0EADA95B6D48 wds:Q58217077-A16A62D0-81F7-466D-B284-FAD67CCBC008 wds:Q58217077-D4BDDB7A-CF13-44F4-B248-434B82F42D6C wds:Q58217077-EB18217B-2051-4811-BA28-4C036E0BA9C1 wds:Q58217077-F63E9EB0-A2EE-4F2D-879E-53C3C700E56A wds:Q58217077-FAE99E89-B6B0-4726-B710-6AB9DB074804
author	James Scott Dunlop Denis Burgarella Douglas Scott Rob Ivison Joaquin Vieira Javier Álvarez-Márquez Lorenzo Moncelsi Julie Wardlow Duncan Farrah Guilaine Lagache Lucia Marchetti Matthieu Béthermin Luca Conversi Georgios Magdis Alberto Franceschini
title	wds:Q58217077-DDD9FC9D-9BCC-4E76-A16B-DA6AA19AA6CB
title	HerMES: current cosmic infrared background estimates can Be explained by known galaxies and their faint companions at z < 4 (en)
page(s)	wds:Q58217077-41526978-BA5B-476B-983B-E9935AC7DDB1
page(s)	22
Internet Archive ID	wds:Q58217077-C4F2457B-8257-4C2A-AFA0-9AB41DCC17B7
Internet Archive ID	arxiv-1505.06242
instance of	wds:Q58217077-B59CEA65-FB42-490D-8BDF-5E554877CE69
instance of	scholarly article
published in	wds:Q58217077-96D6CE26-8948-42EC-A93D-589EF5A0DD78
full work available at URL	wds:Q58217077-DF982DF0-5FEF-41AA-AD71-E59667648B48
published in	Letters of the Astrophysical Journal
full work available at URL	https://iopscience.iop.org/article/10.1088/2041-8205/809/2/L22/pdf
issue	wds:Q58217077-91A9A5C3-5A49-4224-9200-566E3480DF8D
volume	wds:Q58217077-52560720-4EB4-4821-BE7D-789685C30D33
issue	2
volume	809
DOI	wds:Q58217077-70ABF1CB-ABD6-41AA-8BDD-C03FA271054B
DOI	http://dx.doi.org/10.1088/2041-8205/809/2/L22
DOI	10.1088/2041-8205/809/2/L22
arXiv ID	wds:Q58217077-EC453EE6-D748-4B7B-8471-BE18C7E78F2F
arXiv ID	1505.06242
ADS bibcode	wds:Q58217077-E237DBC4-C209-46C0-9813-91E736BA40EA
ADS bibcode	2015ApJ...809L..22V

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