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Por favor, use este identificador para citar o enlazar a este item: http://hdl.handle.net/10261/20240
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dc.contributor.authorNakos, Th.-
dc.contributor.authorBaes, M.-
dc.contributor.authorAlonso-Herrero, A.-
dc.contributor.authorLabiano, Álvaro-
dc.date.accessioned2010-01-21T12:05:58Z-
dc.date.available2010-01-21T12:05:58Z-
dc.date.issued2009-09-
dc.identifier.citationNew Astronomy Reviews 53/7-10): 175-178 (2009)en_US
dc.identifier.issn1387-6473-
dc.identifier.urihttp://hdl.handle.net/10261/20240-
dc.description4 pages, 1 figure, 2 tables.-- Pre-print archive.en_US
dc.description.abstractThe James Webb Space Telescope (JWST), due to launch in 2014, shall provide an unprecedented wealth of information in the near and mid-infrared wavelengths, thanks to its high-sensitivity instruments and its 6.5 m primary mirror, the largest ever launched into space. NIRSpec and MIRI, the two spectrographs onboard JWST, will play a key role in the study of the spectral features of Active Galactic Nuclei in the 0.6–28 μm wavelength range. This article aims at presenting an overview of the possibilities provided by these two instruments, in order to prepare the astronomical community for the JWST era.en_US
dc.description.sponsorshipThe MIRI European Consortium thanks the following National Funding Agencies for their support of the MIRI: Belgian Science Policy Office, Centre Nationale D’Etudes Spatiales, Danish National Space Centre, Deutsches Zentrum fur Luftund Raumfahrt, Enterprise Ireland, Ministerio De Education y Ciencia, Nova, Science and Technology Facilities Council, Swiss Space Office, Swedish National Space Board.en_US
dc.format.extent198495 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoengen_US
dc.publisherElsevieren_US
dc.rightsopenAccessen_US
dc.subjectTechniques: spectroscopicen_US
dc.subjectQuasars: generalen_US
dc.subjectGalaxies: activeen_US
dc.subjectGalaxies: starbursten_US
dc.subjectEarly Universeen_US
dc.titleStudying the spectral properties of Active Galactic Nuclei in the JWST eraen_US
dc.typeartículoen_US
dc.identifier.doi10.1016/j.newar.2009.08.008-
dc.description.peerreviewedPeer revieweden_US
dc.relation.publisherversionhttp://dx.doi.org/10.1016/j.newar.2009.08.008en_US
dc.type.coarhttp://purl.org/coar/resource_type/c_6501es_ES
item.languageiso639-1en-
item.fulltextWith Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
item.grantfulltextopen-
item.openairetypeartículo-
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