dc.contributorInstitut Polytechnique des Sciences Avancées IPSA
dc.contributorUniv. Lille 1
dc.contributorSternberg astronomical institute
dc.contributorIndian Institute of Astrophysics
dc.contributorNorth America and RECON
dc.contributorObservatoire des Baronnies Provencales
dc.contributorPuig d'Agulles
dc.contributorHigh-school Liceo G.Galilei
dc.contributorLagrange
dc.contributorObservatoire Midi Pyrenées
dc.contributorObservatoire du Pic des Fees
dc.contributorVoronezh State University
dc.contributorCollege Hill
dc.contributorAssociation Andromede Observatoire de Marseille
dc.contributorClub Eclipse
dc.contributorCommission des observations planétaires
dc.contributorObservatório Nacional MCTI
dc.contributorNaperville
dc.contributorObservatoire de Dax
dc.contributorInternational Occultation Timing Association (IOTA)
dc.contributorFessenkov Astrophysical Institute
dc.contributorGiaGa Observatory
dc.contributorAmerican Association of Variable Star Observers (AAVSO)
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorKuriwa Observatory
dc.contributorUniversity of Athens University Campus
dc.contributorKourovskaya observatory of the Ural Federal University
dc.contributorCentral Astronomical Observatory of the Russian Academy of Sciences
dc.contributorSocietá Astronomica Ticinese (CH)
dc.contributorEuropean Section
dc.contributorArchenhold-Observatory
dc.contributorRokycany Observatory
dc.contributorClub d'astronomie d'Antony
dc.contributorEgeskov Observatory
dc.contributorSociété Astronomique de Tunisie
dc.contributorHellenic Amateur Astronomy Association
dc.contributorInternational Occultation Timing Association
dc.contributorAndres Bello Astronomical Complex
dc.contributorVenezuelan Society of Amateur Astronomers
dc.contributorUniversidade Estadual do Oeste do Paran a (Unioeste)
dc.contributorPolo Astronmico Casimiro Montenegro Filho/FPTI-BR
dc.contributorResearch Institute Nikolaev Astronomical Observatory
dc.contributorObservatory Rokycany
dc.contributorUniversity of Siena
dc.contributorSalvia Observatory
dc.contributorSociété d'Astronomie de Rennes
dc.contributorUniversidade Federal do Rio de Janeiro (UFRJ)
dc.contributorBucharest Observatory
dc.contributorCanberra Astronomical Society
dc.contributorUniversity of Applied Sciences
dc.contributorAstronomie Stiftung Trebur
dc.contributorNyrola Observatory
dc.contributorTangra Observatory
dc.contributorAmiral Vasile Urseanu Observatory
dc.contributorWest Park Observatory
dc.contributorGroupement Astronomique Populaire de la Région d'Antibes
dc.contributorWellington Astronomical Society
dc.contributorAssociation Club Eclipse et club Albiréo78
dc.contributorRoyal Astronomical Society of New Zealand
dc.contributorObservatoire de Vesqueville
dc.contributorNational Aviation University
dc.contributorImpasse de l'Observatoire
dc.contributorSAF groupe Alsace
dc.contributorEuropean Section (IOTAES)
dc.date.accessioned2018-12-11T16:53:00Z
dc.date.available2018-12-11T16:53:00Z
dc.date.created2018-12-11T16:53:00Z
dc.date.issued2018-03-01
dc.identifierMonthly Notices of the Royal Astronomical Society, v. 474, n. 4, p. 4730-4739, 2018.
dc.identifier1365-2966
dc.identifier0035-8711
dc.identifierhttp://hdl.handle.net/11449/170932
dc.identifier10.1093/mnras/stx2957
dc.identifier2-s2.0-85045988470
dc.identifier2-s2.0-85045988470.pdf
dc.description.abstractDuring the 2014-2015 mutual events season, the Institut de Mécanique Céleste et de Calcul des Éphémérides (IMCCE), Paris, France, and the Sternberg Astronomical Institute (SAI), Moscow, Russia, led an international observation campaign to record ground-based photometric observations of Galilean moon mutual occultations and eclipses.We focused on processing the complete photometric observations data base to compute new accurate astrometric positions. We used our method to derive astrometric positions from the light curves of the events. We developed an accurate photometric model of mutual occultations and eclipses, while correcting for the satellite albedos, Hapke's light scattering law, the phase effect, and the limb darkening. We processed 609 light curves, and we compared the observed positions of the satellites with the theoretical positions from IMCCE NOE-5-2010-GAL satellite ephemerides and INPOP13c planetary ephemeris. The standard deviation after fitting the light curve in equatorial positions is ±24 mas, or 75 km at Jupiter. The rms (O-C) in equatorial positions is ±50 mas, or 150 km at Jupiter.
dc.languageeng
dc.relationMonthly Notices of the Royal Astronomical Society
dc.relation2,346
dc.relation2,346
dc.rightsAcesso aberto
dc.sourceScopus
dc.subjectAstronomical data bases: miscellaneous
dc.subjectEclipses
dc.subjectEphemerides
dc.subjectOccultations
dc.subjectPlanets and satellites: general
dc.subjectTechniques: photometric
dc.titleThe PHEMU15 catalogue and astrometric results of the Jupiter's Galilean satellite mutual occultation and eclipse observations made in 2014-2015
dc.typeArtículos de revistas


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