J/A+AS/125/399ivo://CDS.VizieR/J/A+AS/125/399CDSArlot J.E.Ruatti C.Thuillot W.Arsenijevic J.Baptista R.,Barroso Jr. J.Bauer C.Berthier J.Blanco C.Bouchet P.,Bourgeois J.Bulder H.J.J.Burchi R.Cano J.A.Casas R.Chauvet F.,Chis D.Colas F.Colin J.D'Ambrosio V.De Angelis G.,De Benedetto G.Denzau H.Desbats J.M.Descamps P.Dipaolantonio A.,Dumitrescu A.Farcas L.Federspiel M.Flatres T.Froeschle M.,Gherega O.Gomez-Forrellad J.M.Guarro J.Hainaut O.Horvat A.,Helmer G.Hube D.Ito Y.Kidger M.Lecacheux J.Le Campion J.F.,Le Floch J.C.Mallama A.Martin B.E.Mellilo J.F.Meyer C.,Molau S.Montignac G.Morando B.Nicolet B.Nitschelm B.,Oprescu G.Piersimoni A.Przewozny D.Protitch-Benishek V.,Rapaport M.Riou A.Sacre J.J.Sevre F.Shkodrov V.Souchay J.,Takami H.Taylor R.Tholen D.J.Turcu V.Vasundhara R.Vidal J.,Vu D.T.White G.Wilds R.P.1997-12-09T18:42:38Z1997-12-09T19:42:34ZCDS support team

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

cds-question@unistra.frsolar-system-planetsoccultationIn this paper, all the light-curves obtained during the PHEMU91 campaign of observations of the mutual phenomena of the Galilean satellites are presented. These observations give accurate astrometric positions of major interest for dynamical studies of the motion of the Galilean satellites. The aim of this work is to give observational data directly usable for theoretical studies. We made 374 observations of 111 mutual events from 56 sites. The accuracy of each observation has been deduced from a comparison with the theoretical predictions. For each observation, information is given about the telescope, the receptor, the site and the observational conditions. Other data as well as the data of the lightcurves themselves are available on the server: ftp://ftp.bdl.fr/pub/NSDC/jupiter/pheno_mut/19911997A&AS..125..399Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/125/399CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/314/312 : Galilean satellites mutual events in 1997 (Arlot 1996)J/A+AS/115/295 : Astrometry of outer Jovian satellites (Hernius+, 1996)J/other/KFNT/15.483 : Positions of Thebe and Amalthea (Ledovskaya+ 1999)J/A+A/383/724 : 1999-2000 CCD obs. of inner Jovian moons (Kulyk+, 2002)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/125/399https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/125/399http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/125/399https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/125/399https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/125/399http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/125/399GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+AS/125/399/table2aObserved mutual eventsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintDateGregorian date of the phenomenontime.epochS1First satellite involvedmeta.id.part;meta.maincharPhe[OE] Type of phenomenon (1)meta.notecharS2Second satellite involvedmeta.id.part;meta.maincharType[anpape] Type of phenomenon (2)meta.notecharTB1Predicted hour of the beginning of the event (UTC) with E-2 theorytime.epochTM1Predicted hour of the maximum of the event (UTC) with E-2 theorytime.epochTE1Predicted hour of the end of the event (UTC) with E-2 theorytime.epochMdrop1Magnitude drop with E-2 theorymagphot.mag;arith.difffloatTB2Predicted hour of the beginning of the event (UTC) with E-3 theorytime.epochTM2Predicted hour of the maximum of the event (UTC) with E-3 theorytime.epochTE2Predicted hour of the end of the event (UTC) with E-3 theorytime.epochMdrop2Magnitude drop with E-3 theorymagphot.mag;arith.difffloatTB3Predicted hour of the beginning of the event (UTC) with G-5 theorytime.epochTM3Predicted hour of the maximum of the event (UTC) with G-5 theorytime.epochTE3Predicted hour of the end of the event (UTC) with G-5 theorytime.epochMdrop3Magnitude drop with G-5 theorymagphot.mag;arith.difffloatTB4Predicted hour of the beginning of the event (UTC) with G-5 theory (3)time.epochTM4Predicted hour of the maximum of the event (UTC) with G-5 theory (3)time.epochTE4Predicted hour of the end of the event (UTC) with G-5 theory (3)time.epochMdrop4Magnitude drop with G-5 theory (3)magphot.mag;arith.difffloatDistDistance from the satellites to the center of Jupiter in Jovian radii.pos.distancefloatJ/A+AS/125/399/table2bSite of observation of the mutual eventsPhenPhenomenonmeta.codecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintDateObservation datetime.epochn_Phen[apb] Note when two phenomenons occur at the same date (1)meta.notecharSiteName of the site of observationmeta.id;instr.obstycharTMIN? Hour (UTC) of the minimum of light observedtime.epochLflux? Lightflux drop in arbitrary unitsphot.flux;arith.ratiofloatC-O? Calculated minus Observed time computed with the G-5 predictionsstat.fit.omc;timeintInst[TL] Code for the instrument used (2)meta.notecharApertAperture of the instrument in centimeters (for some instruments)cmphys.size;instrfloatReceptCode for the receptormeta.codecharEJupElevation of Jupiter upon the horizondegpos.az.altintESunElevation of the Sun upon the horizondegpos.az.altintObsCond[1/3]? Conditions of observation code (3)meta.note;obsintFilterCode for the filtermeta.code;instr.filtercharIntTime? Time of integrationstime.duration;obs.exposurefloatSize? Size of the diaphragm or window (CCD)arcsecinstr.fovfloatn_Size[x] x when two lengths for a rectangular CCD windowmeta.notecharSize2? Second length for a rectangular CCD windowarcsecinstr.fovintOrderOrder number of satellites in diaphragm, i.e. the satellites, the global magnitude drop of which was observedobs.paramchare_TMINs? Uncertainty on the observed time of the minimum of lightsstat.errorinte_Lflux? Uncertainty on the lightflux dropstat.errorfloat