=============================================================================== File: 1990-1992_J1-4_aksnes.data.txt =============================== Contents: The paper analyses 213 light curves of 86 mutual phenomena. About 80% of the data have been taken from Phemu91 NSDC data base, while 40 light curves were observed by the authors or communicated to them. The data are relative positions of observed satellites deduced from the light curves. References: Kaas, A.A., Aksnes K., Franklin F., Lieske J.H.: 1999, Astrometry from Mutual Phenomena of the Galilean Satellites in 1990-1992, Astron. J. 117, 1933-1941 Format: The format of the data is the one of table 1 in the paper given in the references above. Codes for observatories: ESO: European Southern Obs. Chile BNZ: Adams Obs. Blenheim N. Zealand BMD: Bowie Maryland USA LOW: Lowell Obs. Flagstaff Ariz. USA GEA: Grup d'Estuds Astron. No. Spain VIA: Victoria NSW Australia RCI: Reggio Calabria Italy PIC: Pic du Midi France ORM: Oak Ridge Obs. Mass. USA RIO: Rio de Janeiro Brazil CAT: Catania Astrophys. Obs. Sicily BOR: Bordeaux Univ. Obs. France TOK: Tokyo Obs. Japan MEU: Meudon Obs. France NIC: Nice Obs. France CNR: Cluj-Napoca Obs. Romania TER: Collurania Obs. Teramo Italy SSA: Siding Spring Obs. Australia CAF: Calern, Cote d'Azur France MKH: Mauna Kea, Hawaii KAV: Vainu Bappu Obs. Kavalur India TOC: Toronto Ontario Canada PRI: Providence Rhode Island USA BRB: Brasopolis Brazil HAN: Harastua Norway DNC: Durham North Carolina USA OHP: Obs. Haute-Provence France BER: Berlin Germany PAR: Paris Obs. France HEG: Heuweiler Germany BSP: Barcelona Spain ESS: Essen Germany KAK: Kakuda Japan HNY: Holtsville New York USA ZNL: Zoetermeer Netherlands TMR: Timisoara Romania SFC: San Francisco Cal. USA TPK: Topeka Kansas USA DAC: Devon Ast. Obs. Alberta Canada BEL: Belgrade Obs. Serbia ===============================================================================