J/MNRAS/371/1503ivo://CDS.VizieR/J/MNRAS/371/1503doi:10.26093/cds/vizier.73711503CDSMarconi M.Cignoni M.Di Criscienzo M.Ripepi V.Castelli F.,Musella I.Ruoppo A.2024-07-03T20:13:58Z2012-04-09T14:56:34ZCDS support team

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

cds-question@unistra.frvariable-starsastronomical-modelsThe luminosities and effective temperatures, as well as the whole bolometric light curves of non-linear convective RR Lyrae models with 0.0001<=Z<=0.006, are transformed into the Sloan Digital Sky Survey (SDSS) photometric system. The obtained ugriz light curves, mean magnitudes and colours, pulsation amplitudes and colour-colour loops are shown and analytical relations connecting pulsational to intrinsic stellar parameters, similar to the ones currently used in the JohnsonCousins filters, are derived. Finally, the behaviour in the colour-colour planes is compared with available observations in the literature and possible systematic uncertainties affecting this comparison are discussed.2006MNRAS.371.1503Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/371/1503CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/121/327 : RR Lyr pulsational model (Bono+ 1997)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/371/1503https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/371/1503http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/371/1503https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/371/1503https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/371/1503http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/371/1503GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/MNRAS/371/1503/mode_0Intensity-averaged mean magnitudes and pulsation amplitudes for the RR Lyr stars in the fundamental moderecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZ[0.0001/0.004] Metallicity (values 10^-4^, 4x10^-4^, 10^-3^, 4x10^-3^)phys.abund.ZfloatM[0.65/0.80] Mass of starsolMassphys.massfloatlogL[1.51/1.91] Bolometric luminositylog(solLum)phys.luminosityfloatTeff[5800/7300] Effective temperatureKphys.temperature.effectiveintP[0.21/1.15] Pulsation perioddtime.periodfloat<umag>Mean magnitude in the SDSS u-bandmagphot.mag;em.opt.Ufloat<gmag>Mean magnitude in the SDSS g-bandmagphot.mag;em.opt.Bfloat<rmag>Mean magnitude in the SDSS r-bandmagphot.mag;em.opt.Rfloat<imag>Mean magnitude in the SDSS i-bandmagphot.mag;em.opt.Ifloat<zmag>Mean magnitude in the SDSS z-bandmagphot.mag;em.opt.IfloatuAmpAmplitude in the SDSS u-bandmagsrc.var.amplitudefloatgAmpAmplitude in the SDSS g-bandmagsrc.var.amplitudefloatrAmpAmplitude in the SDSS r-bandmagsrc.var.amplitudefloatiAmpAmplitude in the SDSS i-bandmagsrc.var.amplitudefloatzAmpAmplitude in the SDSS z-bandmagsrc.var.amplitudefloatJ/MNRAS/371/1503/mode_1Intensity-averaged mean magnitudes and pulsation amplitudes for the RR Lyr stars in the first overtone moderecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZ[0.0001/0.004] Metallicity (values 10^-4^, 4x10^-4^, 10^-3^, 4x10^-3^)phys.abund.ZfloatM[0.65/0.80] Mass of starsolMassphys.massfloatlogL[1.51/1.91] Bolometric luminositylog(solLum)phys.luminosityfloatTeff[5800/7300] Effective temperatureKphys.temperature.effectiveintP[0.21/1.15] Pulsation perioddtime.periodfloat<umag>Mean magnitude in the SDSS u-bandmagphot.mag;em.opt.Ufloat<gmag>Mean magnitude in the SDSS g-bandmagphot.mag;em.opt.Bfloat<rmag>Mean magnitude in the SDSS r-bandmagphot.mag;em.opt.Rfloat<imag>Mean magnitude in the SDSS i-bandmagphot.mag;em.opt.Ifloat<zmag>Mean magnitude in the SDSS z-bandmagphot.mag;em.opt.IfloatuAmpAmplitude in the SDSS u-bandmagsrc.var.amplitudefloatgAmpAmplitude in the SDSS g-bandmagsrc.var.amplitudefloatrAmpAmplitude in the SDSS r-bandmagsrc.var.amplitudefloatiAmpAmplitude in the SDSS i-bandmagsrc.var.amplitudefloatzAmpAmplitude in the SDSS z-bandmagsrc.var.amplitudefloat