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The IUE flux scale

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dc.contributor.author González-Riestra, Rosario
dc.date.accessioned 2017-02-04T16:25:05Z
dc.date.available 2017-02-04T16:25:05Z
dc.date.issued 1998
dc.identifier.citation Gonzalez-Riestra, R. (1998). The IUE Flux Scale. European Space Agency, (Special Publication) ESA SP, 413, 707 spa
dc.identifier.issn 03796566
dc.identifier.uri http://hdl.handle.net/11268/6195
dc.description.abstract One of the by-products of the IUE Final Archive has been the redefinition of the Ultraviolet Flux Scale. The method followed is a two stages process in which the relative and the absolute flux scales are derived separately. The relative flux scale is based on White Dwarf models, as is the case for other space experiments (HST, HUT). The zero point, which defines the Absolute Flux scale is set by the OAO-2 measurements in the band 2100-2300 Å. spa
dc.description.sponsorship Sin financiación spa
dc.language.iso eng spa
dc.title The IUE flux scale spa
dc.type article spa
dc.description.impact 0.182 JCR (1998) Q3, 16/28 Aerospace Engineering & Technology spa
dc.rights.accessRights openAccess en
dc.subject.uem Astrofísica spa
dc.subject.uem Astronomía spa
dc.subject.uem Vehículos espaciales spa
dc.subject.unesco Astrofísica spa
dc.subject.unesco Astronomía spa
dc.subject.unesco Vehículo espacial spa
dc.description.filiation UEM spa
dc.relation.publisherversion http://sdc.cab.inta-csic.es/ines/docs/iue_flux.pdf spa
dc.peerreviewed Si spa


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