J/A+AS/106/327ivo://CDS.VizieR/J/A+AS/106/327CDSNOEL F.1997-12-09T17:26:55Z1997-12-09T18:26:51ZCDS support team

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

cds-question@unistra.frthe-sunastrometry(no description available)1994A&AS..106..327Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/106/327CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/102/11 : Astrolabe observations of the Sun in 1990-1992 (Noel 1993)J/A+AS/106/441 : Second catalogue of Santiago (Noel, 1994)J/A+AS/113/131 : Observations of the Sun during 1994 (Noel, 1995)J/A+AS/132/195 : Astrolabe observations of the Sun in 1995-1997 (Noel 1998)J/A+A/375/614 : Astrolabe observations of the Sun in 1990-2000 (Noel, 2001)J/A+A/384/650 : CCD solar diameter measurements in 1999-2000 (Penna+, 2002)J/A+AS/135/227 : Solar diameter observations in 1997-1998 (Jilinski+, 1999)J/A+AS/143/265 : Solar diameter observations in 1998-1999 (Puliaev+, 2000)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/106/327https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/106/327http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/106/327https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/106/327https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/106/327http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/106/327GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+AS/106/327/table2Astrolabe of Santiago: results of Sun observations, 1993. Zenith distance = 30 degrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintDateDate of observation (year, month, day)time.epochintMJDModiufied julian daydtime.epochdoubleEUBZenith distance residual given by the observation of the Sun east upper borderarcsecstat.fit.residual;pos.az.zdfloatELBZenith distance residual given by the observation of the Sun east lower borderarcsecstat.fit.residual;pos.az.zdfloatWLB[]? Zenith distance residual given by the observation of the Sun west lower borderarcsecstat.fit.residual;pos.az.zdfloatWUB[]? Zenith distance residual given by the observation of the Sun west upper borderarcsecstat.fit.residual;pos.az.zdfloatdAlpha[]? Right ascension (observed-ephemeris)spos.eq.ra;arith.difffloate_dAlpha[]? rms uncertainty on dAlphasstat.errorfloatY[]? dz + d{delta} cos S, where dz = Zenith distance (observed-adopted), d{delta} = Declination (observed-ephemeris), S = sun paralactic angle (Chollet & Noel, 1993)arcsecpos.angDistancefloatdD[]? Sun semi-diameterarcsecphys.angSize;srcfloate_dD[]? rms uncertainty on Y and dDarcsecstat.errorfloatDR[]? Observed Sun apparent semi-diameter reduced to the geocenter and to the astronomical unitarcsecphys.angSize;srcfloatJ/A+AS/106/327/table3Astrolabe of Santiago: results of Sun observations, 1993. Zenith distance = 60 degrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintDateDate of observation (year, month, day)time.epochintMJDModiufied julian daydtime.epochdoubleEUBZenith distance residual given by the observation of the Sun east upper borderarcsecstat.fit.residual;pos.az.zdfloatELBZenith distance residual given by the observation of the Sun east lower borderarcsecstat.fit.residual;pos.az.zdfloatWLB[]? Zenith distance residual given by the observation of the Sun west lower borderarcsecstat.fit.residual;pos.az.zdfloatWUB[]? Zenith distance residual given by the observation of the Sun west upper borderarcsecstat.fit.residual;pos.az.zdfloatdAlpha[]? Right ascension (observed-ephemeris)spos.eq.ra;arith.difffloate_dAlpha[]? rms uncertainty on dAlphasstat.errorfloatY[]? dz + d{delta} cos S, where dz = Zenith distance (observed-adopted), d{delta} = Declination (observed-ephemeris), S = sun paralactic angle (Chollet & Noel, 1993)arcsecpos.angDistancefloatdD[]? Sun semi-diameterarcsecphys.angSize;srcfloate_dD[]? rms uncertainty on Y and dDarcsecstat.errorfloatDR[]? Observed Sun apparent semi-diameter reduced to the geocenter and to the astronomical unitarcsecphys.angSize;srcfloat