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dc.contributor.authorGonzález-Nuevo González, Joaquín
dc.contributor.authorDe Zotti, Gianfranco
dc.contributor.authorAndreani, Paola
dc.contributor.authorBarton, Emma J.
dc.contributor.authorBertoldi, Frank
dc.contributor.authorBirkinshaw, Mark
dc.contributor.authorBonavera, Laura
dc.contributor.authorButtiglione, Mara
dc.contributor.authorCooke, Jeff
dc.contributor.authorCooray, Asantha
dc.contributor.authorDanese, Giovanni
dc.contributor.authorDunne, Loretta
dc.contributor.authorEales, Stephen
dc.contributor.authorFan, Lulu
dc.contributor.authorJarvis, Matthew J.
dc.contributor.authorKlöckner, Hans-Rainer
dc.contributor.authorHatziminaoglou, Evanthia
dc.contributor.authorHerranz Muñoz, Diego 
dc.contributor.authorLópez-Caniego Alcarria, Marcos
dc.contributor.authorVerma, Aprajita
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2023-03-16T13:56:53Z
dc.date.available2023-03-16T13:56:53Z
dc.date.issued2010
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.urihttps://hdl.handle.net/10902/28220
dc.description.abstractTo investigate the poorly constrained sub-mm counts and spectral properties of blazars we searched for these in the Herschel-ATLAS (H-ATLAS) science demonstration phase (SDP) survey catalog. We cross-matched 500 μm sources brighter than 50 mJy with the FIRST radio catalogue. We found two blazars, both previously known. Our study is among the first blind blazar searches at sub-mm wavelengths, i.e., in the spectral regime where little is still known about the blazar SEDs, but where the synchrotron peak of the most luminous blazars is expected to occur. Our early results are consistent with educated extrapolations of lower frequency counts and question indications of substantial spectral curvature downwardsand of spectral upturns at mm wavelengths. One of the two blazars is identified with a Fermi/LAT Υ-ray source and a WMAP source. The physical parameters of the two blazars are briefly discussed. These observations demonstrate that the H-ATLAS survey will provide key information aboutthe physics of blazars and their contribution to sub-mm counts.es_ES
dc.description.sponsorshipWe are grateful to the referee, P. Padovani, for very useful comments. Thanks are due to the PACO collaboration for having made available the data on the 2 blazars. M.M. and L.B. thanks the staff at the Australia Telescope Compact Array site, Narrabri (NSW), for the valuable support they provide in running the telescope. Work partially supported by the Italian Space Agency (contract I/016/07/0 "COFIS'' and ASI/INAF Agreement I/072/09/0 for the Planck LFI Activity of Phase E2). This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.es_ES
dc.format.extent4 p.es_ES
dc.language.isoenges_ES
dc.publisherEDP Scienceses_ES
dc.rights© ESO, 2010es_ES
dc.sourceAstronomy and Astrophysics, 2010, 518, L38es_ES
dc.subject.otherBL Lacertae objects: generales_ES
dc.subject.otherQuasars: generales_ES
dc.subject.otherSubmillimeter: generales_ES
dc.titleHerschel-ATLAS: Blazars in the science demonstration phase fieldes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1051/0004-6361/201014637es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1051/0004-6361/201014637
dc.type.versionpublishedVersiones_ES


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