@article {28396,
	title = {The PHEMU15 catalogue and astrometric results of the Jupiter{\textquoteright}s Galilean satellite mutual occultation and eclipse observations made in 2014-2015},
	volume = {474},
	year = {2018},
	month = {2018/03/1},
	pages = {4730 - 4739},
	abstract = {During the 2014-2015 mutual events season, the Institut de M{\'e}canique C{\'e}leste et de Calcul des {\'E}ph{\'e}m{\'e}rides (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{\textquoteright}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 {\textpm}24 mas, or 75 km at Jupiter. The rms (O-C) in equatorial positions is {\textpm}50 mas, or 150 km at Jupiter.},
	keywords = {astronomical data bases: miscellaneous, eclipses, Ephemerides, Occultations, planets and satellites: general, techniques: photometric},
	isbn = {0035-8711},
	url = {https://ui.adsabs.harvard.edu/abs/2018MNRAS.474.4730S},
	author = {Saquet, E. and Emelyanov, N. and Robert, V. and Arlot, J. -E. and Anbazhagan, P. and Bailli{\'e}, K. and Bardecker, J. and Berezhnoy, A. A. and Bretton, M. and Campos, F. and Capannoli, L. and Carry, B. and Castet, M. and Charbonnier, Y. and Chernikov, M. M. and Christou, A. and Colas, F. and Coliac, J. -F. and Dangl, G. and Dechambre, O. and Delcroix, M. and Dias-Oliveira, A. and Drillaud, C. and Duchemin, Y. and Dunford, R. and Dupouy, P. and Ellington, C. and Fabre, P. and Filippov, V. A. and Finnegan, J. and Foglia, S. and Font, D. and Gaillard, B. and Galli, G. and Garlitz, J. and Gasmi, A. and Gaspar, H. S. and Gault, D. and Gazeas, K. and George, T. and Gorda, S. Y. and Gorshanov, D. L. and Gualdoni, C. and Guhl, K. and Halir, K. and Hanna, W. and Henry, X. and Herald, D. and Houdin, G. and Ito, Y. and Izmailov, I. S. and Jacobsen, J. and Jones, A. and Kamoun, S. and Kardasis, E. and Karimov, A. M. and Khovritchev, M. Y. and Kulikova, A. M. and Laborde, J. and Lainey, V. and Lavayssiere, M. and Le Guen, P. and Leroy, A. and Loader, B. and Lopez, O. C. and Lyashenko, A. Y. and Lyssenko, P. G. and Machado, D. I. and Maigurova, N. and Manek, J. and Marchini, A. and Midavaine, T. and Montier, J. and Morgado, B. E. and Naumov, K. N. and Nedelcu, A. and Newman, J. and Ohlert, J. M. and Oksanen, A. and Pavlov, H. and Petrescu, E. and Pomazan, A. and Popescu, M. and Pratt, A. and Raskhozhev, V. N. and Resch, J. -M. and Robilliard, D. and Roschina, E. and Rothenberg, E. and Rottenborn, M. and Rusov, S. A. and Saby, F. and Saya, L. F. and Selvakumar, G. and Signoret, F. and Slesarenko, V. Y. and Sokov, E. N. and Soldateschi, J. and Sonka, A. and Soulie, G. and Talbot, J. and Tejfel, V. G. and Thuillot, W. and Timerson, B. and Toma, R. and Torsellini, S. and Trabuco, L. L. and Traverse, P. and Tsamis, V. and Unwin, M. and Abbeel, F. Van Den and Vandenbruaene, H. and Vasundhara, R. and Velikodsky, Y. I. and Vienne, A. and Vilar, J. and Vugnon, J. -M. and Wuensche, N. and Zeleny, P.}
}
