J/A+A/423/983ivo://CDS.VizieR/J/A+A/423/983doi:10.26093/cds/vizier.34230983CDSMutschke H.Andersen A.C.Jaeger A.C.Henning T.Braatz A.2004-10-16T22:28:57Z2004-10-16T22:28:52ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frsolar-systemchemical-abundancesWe have used different spectroscopic techniques to obtain a consistent quantitative absorption spectrum of a sample of meteoritic nano-diamonds in the wavelength range from the vacuum ultraviolet (0.12um) to the far infrared (100um). The nano-diamonds have been isolated by a chemical treatment from the Allende meteorite (Braatz et al. 2000, Meteorit. Planet. Sci., 35, 75). Electron energy loss spectroscopy (EELS) extends the optical measurements to higher energies and allows the derivation of the optical constants (n & k) by Kramers-Kronig analysis.2004A&A...423..983Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/423/983CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/423/983https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/423/983http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/423/983https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/423/983https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/423/983http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/423/983GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/423/983/table3Table of the real (n) and imaginary (k) parts of the complex refractive index depending on wavelengthrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelengthumem.wldoublenReal part of refractive indexobs.atmos.refractAnglefloatkImaginary part of refractive indexobs.atmos.refractAnglefloat