J/A+A/527/A146ivo://CDS.VizieR/J/A+A/527/A146doi:10.26093/cds/vizier.35270146CDSChadid M.Perini C.Bono G.Auvergne M.Baglin A.Weiss W.W.,Deboscher J.2017-06-21T08:22:17Z2011-02-14T08:47:31ZCDS support team

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

cds-question@unistra.frvariable-starsspectroscopyThe CoRoT - Convection Rotation and Planetary Transits - space mission provides a unique opportunity to monitor RR Lyrae stars with excellent time-sampling, unprecedented photometric precision, and a long time base of 150 days. The pulsation characteristics of RR Lyrae stars rely on robust physics, but we still lack a firm quantitative understanding of the physical mechanisms driving the Blazhko modulation and the long-term changes in their pulsation behavior. We use the high- precision space data of an unknown RR Lyrae star CoRoT ID 0105288363 observed during a second long run centered on the Galaxy -LRc02-, to improve our understanding of the pulsation properties of RR Lyrae stars.2011A&A...527A.146Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/527/A146CatalogResearchIsServedByTAP VizieR generic servicerelated-toB/corot : CoRoT observation log (CoRoT, 2009)J/A+A/510/A39 : CoRoT light curves of V1127 Aql (Chadid+, 2010)J/A+A/520/A108 : CoRoT 101128793 light curves (Poretti+, 2010)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/527/A146https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/527/A146http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/527/A146https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/527/A146https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/527/A146http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/527/A146GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/527/A146/tableFourier amplitudes, phases, spectral significance and identification of the detected frequencies in the CoRoT data of the star CoRoT ID 0105288363recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintCycle[1/4] Blazhko cycle numbermeta.id;meta.mainintType[A-H] Type of frequency (1)meta.codecharFreqFourier frequencyd**-1em.freqdoubleAmplFourier amplitudemmagsrc.var.amplitudedoublePhasePhaseradtime.phasedoublesigSpectral significancestat.fit.goodnessdoubleIdIdentification of the frequencymeta.notechar