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PACS Evolutionary Probe (PEP) - A Herschel key program

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dc.contributor.authorCava, A.
dc.contributor.authorDomínguez Sánchez, Helena
dc.date.accessioned2023-06-20T03:56:00Z
dc.date.available2023-06-20T03:56:00Z
dc.date.issued2011-08
dc.description© ESO 2011. © EDP Sciences. Artículo firmado por 39 autores. We thank the referee for helpful comments. PACS has been developed by a consortium of institutes led by MPE (Germany) and including UVIE (Austria); KUL, CSL, IMEC (Belgium); CEA, OAMP (France); MPIA (Germany); IFSI, OAP/OAT, OAA/CAISMI, LENS, SISSA (Italy); IAC (Spain). This development has been supported by the funding agencies BMVIT (Austria), ESA-PRODEX (Belgium), CEA/CNES (France), DLR (Germany), ASI (Italy), and CICYT/MCYT (Spain).
dc.description.abstractDeep far-infrared photometric surveys studying galaxy evolution and the nature of the cosmic infrared background are a key strength of the Herschel mission. We describe the scientific motivation for the PACS Evolutionary Probe (PEP) guaranteed time key program and its role within the entire set of Herschel surveys, and the field selection that includes popular multiwavelength fields such as GOODS, COSMOS, Lockman Hole, ECDFS, and EGS. We provide an account of the observing strategies and data reduction methods used. An overview of first science results illustrates the potential of PEP in providing calorimetric star formation rates for high-redshift galaxy populations, thus testing and superseding previous extrapolations from other wavelengths, and enabling a wide range of galaxy evolution studies.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipBMVIT (Austria)
dc.description.sponsorshipESA-PRODEX (Belgium)
dc.description.sponsorshipCEA/CNES (France)
dc.description.sponsorshipDLR (Germany)
dc.description.sponsorshipASI (Italy)
dc.description.sponsorshipComisión Interministerial de Ciencia y Tecnología (CICYT), España
dc.description.sponsorshipMinisterio de Ciencia y Tecnología (MCYT), España
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/31425
dc.identifier.doi10.1051/0004-6361/201117107
dc.identifier.issn0004-6361
dc.identifier.officialurlhttp://dx.doi.org/10.1051/0004-6361/201117107
dc.identifier.relatedurlhttp://www.aanda.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/44688
dc.journal.titleAstronomy & Astrophysics
dc.language.isoeng
dc.publisherEDP Sciencies
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordStar-formation history
dc.subject.keywordDeep-field-south
dc.subject.keywordSimilar-to 3
dc.subject.keywordLuminous infrared galaxies
dc.subject.keywordActive galactic nuclei
dc.subject.keywordHigh-redshift
dc.subject.keywordSubmillimeter galaxies
dc.subject.keywordMassive galaxies
dc.subject.keywordForming galaxies
dc.subject.keywordSpitzer view
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.titlePACS Evolutionary Probe (PEP) - A Herschel key program
dc.typejournal article
dc.volume.number532
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