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dc.contributor.authorHerranz Muñoz, Diego 
dc.contributor.authorGonzález-Nuevo González, Joaquín
dc.contributor.authorClements, David L.
dc.contributor.authorClemens, M.
dc.contributor.authorDe Zotti, Gianfranco
dc.contributor.authorLópez-Caniego Alcarria, Marcos
dc.contributor.authorLapi, A.
dc.contributor.authorDanese, L.
dc.contributor.authorRodighiero, Giulia
dc.contributor.authorFu, H.
dc.contributor.authorCooray, A.
dc.contributor.authorBaes, Maarten
dc.contributor.authorBendo, G. J.
dc.contributor.authorBonavera, Laura
dc.contributor.authorCarrera Troyano, Francisco Jesús 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2022-08-03T08:52:23Z
dc.date.available2022-08-03T08:52:23Z
dc.date.issued2013-01
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.otherAYA2010-21766-C03-01es_ES
dc.identifier.otherCSD2010-00064es_ES
dc.identifier.otherAYA2010-21490-C02-01es_ES
dc.identifier.urihttp://hdl.handle.net/10902/25445
dc.description.abstractWe present the results of a cross-correlation of the Planck Early Release Compact Source catalogue (ERCSC) with the catalogue of Herschel-ATLAS sources detected in the phase 1 fields, covering 134.55 deg2. There are 28 ERCSC sources detected by Planck at 857 GHz in this area. As many as 16 of them are probably high Galactic latitude cirrus; 10 additional sources can be clearly identified as bright, low-z galaxies; one further source is resolved by Herschel as two relatively bright sources; and the last is resolved into an unusual condensation of low-flux, probably high-redshift point sources, around a strongly lensed Herschel-ATLAS source at z = 3.26. Our results demonstrate that the higher sensitivity and higher angular resolution H-ATLAS maps provide essential information for the interpretation of candidate sources extracted from Planck sub-mm maps.es_ES
dc.description.sponsorshipThe Herschel-ATLAS is a project with Herschel, which is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. The H-ATLAS website is http://www.h-atlas.org/. D.H. and M.L.C. acknowledge partial financial support from the Spanish Ministerio de Ciencia e Innovación project AYA2010-21766-C03-01 and the Consolider Ingenio- 2010 Programme project CSD2010-00064. D.H. also acknowledges the Spanish Ministerio de Educación for a José Castillejo’ mobility grant with reference JC2010-0096 and the Astronomy Department at the Cavendish Laboratory for their hospitality during the elaboration of this paper. The Italian group has been supported in part by ASI/INAF agreement No. I/009/10/0 and by INAF through the PRIN 2009 “New light on the early Universe with sub-mm spectroscopy”. F.J.C. acknowledges partial financial support from the Spanish Ministerio de Ciencia e Innovación project AYA2010-21490-C02-01.es_ES
dc.format.extent13 p.es_ES
dc.language.isoenges_ES
dc.publisherEDP Scienceses_ES
dc.rights© ESO 2013es_ES
dc.sourceAstronomy and Astrophysics, 2013, 549, A31es_ES
dc.subject.otherGalaxies: generales_ES
dc.subject.otherGalaxies: evolutiones_ES
dc.subject.otherSubmillimeter: galaxieses_ES
dc.subject.otherCatalogses_ES
dc.subject.otherGravitational lensing: stronges_ES
dc.titleHerschel-ATLAS: Planck sources in the phase 1 fieldses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1051/0004-6361/201219435es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1051/0004-6361/201219435
dc.type.versionpublishedVersiones_ES


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