J/A+A/544/A125ivo://CDS.VizieR/J/A+A/544/A125doi:10.26093/cds/vizier.35440125CDSMolaro P.Monai S.2012-11-10T14:56:05Z2012-08-13T10:09:10ZCDS support team

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

cds-question@unistra.frthe-sunradial-velocityspectroscopyPresent knowledge of the solar spectrum is limited because it is very difficult to observe the integrated solar spectrum at high resolution. The reflected solar light from asteroids has been shown to provide a relatively straightforward integrated and unmodified solar spectrum. We exploit this methodology to improve our knowledge of solar photospheric line positions both in terms of line number and precision with respect to the available solar line atlas.2012A&A...544A.125Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/544/A125CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/129/41 : Fe I line shifts in the Sun (Allende Prieto+ 1998)J/A+AS/131/431 : Accurate wavelengths in Sun spectrum (Allende Prieto+ 1998)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/544/A125https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/544/A125http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/544/A125https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/544/A125https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/544/A125http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/544/A125GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/544/A125/table3Solar lines list positionsMDetails from Allende Prieto 1998meta.ref.urlcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintCeres[4006/6856] Wavelength position from Ceres spectra0.1nmem.wldoubleAP98Wavelength position from Allende Prieto line list (Cat. J/A+AS/131/431)0.1nmem.wldoubleIonElement identificationphys.atmol.ionStagechardRVRadial velocity differencekm/sspect.dopplerVeloc;arith.difffloat