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dc.contributor.authorRigby, E. E.
dc.contributor.authorMaddox, S. J.
dc.contributor.authorDunne, L.
dc.contributor.authorNegrello, M.
dc.contributor.authorSmith, D. J. B.
dc.contributor.authorGonzalez-Nuevo, J.
dc.contributor.authorHerranz Muñoz, Diego 
dc.contributor.authorLópez-Caniego Alcarria, Marcos
dc.contributor.authorAuld, R.
dc.contributor.authorButtiglione, S.
dc.contributor.authorBaes, M.
dc.contributor.authorCava, A.
dc.contributor.authorCooray, A.
dc.contributor.authorClements, D. L.
dc.contributor.authorDariush, A.
dc.contributor.authorDe Zotti, G.
dc.contributor.authorDye, S.
dc.contributor.authorEales, S.
dc.contributor.authorFrayer, D.
dc.contributor.authorFritz, J.
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2023-04-03T13:02:27Z
dc.date.available2023-04-03T13:02:27Z
dc.date.issued2011-08
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966
dc.identifier.urihttps://hdl.handle.net/10902/28441
dc.description.abstractThe Herschel Astrophysical Terahertz Large Area Survey (Herschel-ATLAS) is a survey of 550 deg2 with the Herschel Space Observatory in five far-infrared and submillimetre bands. The first data for the survey, observations of a field 4 × 4 deg2 in size, were taken during the Science Demonstration Phase (SDP), and reach a 5? noise level of 33.5 mJy beam?1 at 250 µm. This paper describes the source extraction methods used to create the corresponding SDP catalogue, which contains 6876 sources, selected at 250 µm, within ?14 deg2. Spectral and Photometric Imaging REciever (SPIRE) sources are extracted using a new method specifically developed for Herschel data and Photodetector Array Camera and Spectrometer (PACS) counterparts of these sources are identified using circular apertures placed at the SPIRE positions. Aperture flux densities are measured for sources identified as extended after matching to optical wavelengths. The reliability of this catalogue is also discussed, using full simulated maps at the three SPIRE bands. These show that a significant number of sources at 350 and 500 µm have undergone flux density enhancements of up to a factor of ?2, due mainly to source confusion. Correction factors are determined for these effects. The SDP data set and corresponding catalogue will be available from www.h-atlas.org.es_ES
dc.description.sponsorshipThe Herschel-ATLAS is a project with Herschel, which is an ESA space observatory with science instruments provided by Europeanled Principal Investigator consortia and with important participation from NASA. The H-ATLAS website is http://www.h-atlas.org/1. The US participants in Herschel-ATLAS acknowledge support provided by NASA through a contract issued from JPL. The Italian group acknowledges partial financial support from ASI/INAF agreement n. I/009/10/0.es_ES
dc.format.extent13 p.es_ES
dc.language.isoenges_ES
dc.publisherOxford University Presses_ES
dc.rightsThis article has been accepted for publication in Monthly notices of the Royal Astronomical Society © 2011 The authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.es_ES
dc.sourceMonthly Notices of the Royal Astronomical Society, 2011, 415(3), 2336-2348es_ES
dc.subject.otherMethods: data analysises_ES
dc.subject.otherCatalogueses_ES
dc.subject.otherSurveyses_ES
dc.subject.otherGalaxies: generales_ES
dc.subject.otherSubmillimetre: galaxieses_ES
dc.titleHerschel-ATLAS: first data release of the Science Demonstration Phase source catalogueses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1111/j.1365-2966.2011.18864.xes_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1111/j.1365-2966.2011.18864.x
dc.type.versionpublishedVersiones_ES


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