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Title:
The PHEMU03 catalogue of observations of the mutual phenomena of the Galilean satellites of Jupiter
Authors:
Arlot, J.-E.; Thuillot, W.; Ruatti, C.; Ahmad, A.; Amossé, A.; Anbazhagan, P.; Andreyev, M.; Antov, A.; Appakutty, M.; Asher, D.; Aubry, S.; Baron, N.; Bassiere, N.; Berthe, M.; Bogdanovski, R.; Bosq, F.; Bredner, E.; Buettner, D.; Buromsky, M.; Cammarata, S.; Casas, R.; Chis, G. D.; Christou, A. A.; Coquerel, J.-P.; Corlan, R.; Cremaschini, C.; Crussaire, D.; Cuypers, J.; Dennefeld, M.; Descamps, P.; Devyatkin, A.; Dimitrov, D.; Dorokhova, T. N.; Dorokhov, N. I.; Dourneau, G.; Dueñas, M.; Dumitrescu, A.; Emelianov, N.; Ferrara, D.; Fiel, D.; Fienga, A.; Flatres, T.; Foglia, S.; Garlitz, J.; Gerbos, J.; Gilbert, R.; Goncalves, R. M. D.; Gonzãles, D.; Gorda, S. Yu.; Gorshanov, D. L.; Hansen, M. W.; Harrington, M.; Irsmambetova, T. R.; Ito, Y.; Ivanova, V.; Izmailov, I. S.; Khovritchev, M. Yu.; Khrutskaya, E. V.; Kieken, J.; Kiseleva, T. P.; Kuppuswamy, K.; Lainey, V.; Lavayssiére, M.; Lazzarotti, P.; Le Campion, J.-F.; Lellouch, E.; Li, Z. L.; Lo Savio, E.; Lou, M.; Magny, E.; Manek, J.; Marinello, W.; Marino, G.; McAuliffe, J. P.; Michelli, M.; Moldovan, D.; Montagnac, S.; Moorthy, V.; Nickel, O.; Nier, J. M.; Noel, T.; Noyelles, B.; Oksanen, A.; Parrat, D.; Pauwels, T.; Peng, Q. Y.; Pizzetti, G.; Priban, V.; Ramachandran, B.; Rambaux, N.; Rapaport, M.; Rapavy, P.; Rau, G.; Sacré, J.-J.; Sada, P. V.; Salvaggio, F.; Sarlin, P.; Sciuto, C.; Selvakumar, G.; Sergeyev, A.; Sidorov, M.; Sorescu, S.; Spampinato, S. A.; Stellmacher, I.; Trunkovsky, E.; Tejfel, V.; Tudose, V.; Turcu, V.; Ugarte, I.; Vantyghem, P.; Vasundhara, R.; Vaubaillon, J.; Velu, C.; Venkataramana, A. K.; Vidal-Sãinz, J.; Vienne, A.; Vilar, J.; Vingerhoets, P.; Vollman, W.
Affiliation:
AA(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France ), AB(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France), AC(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France), AD(Armagh Observatory, Armagh, Northern Ireland, UK), AE(Forum des sciences, Villeneuve d'Ascq, Lille, France), AF(IIA (Indian Institute of Astrophysics), VBO, Kavalur, India), AG(Terskol Observatory, Kabardino-Balkaria, Russia), AH(Rozhen Observatory, Bulgaria), AI(IIA (Indian Institute of Astrophysics), VBO, Kavalur, India), AJ(Armagh Observatory, Armagh, Northern Ireland, UK), AK(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France), AL(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France), AM(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France), AN(Observatoire de l'université de Lille, Lille, France), AO(Rozhen Observatory, Bulgaria), AP(Observatoire de Bordeaux, Floirac, France), AQ(Dolberg, Germany), AR(Chemnitz, Germany), AS(Kiev National University, Kiev, Ukraine), AT(GAC, Catania, Italy), AU(IAC, Tenerife, Spain), AV(Cluj-Napoca, Romania), AW(Armagh Observatory, Armagh, Northern Ireland, UK), AX(C2AHP, Saint-Michel l'observatoire, France), AY(Institutul Astronomic, Bucuresti, Romania), AZ(Observatorio S. Zani, Lumezzane, Italy), BA(Observatoire de Paris, Meudon, France), BB(Royal Observatory of Belgium, Brussels, Belgium), BC(IAP, Paris, France), BD(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France), BE(Pulkovo Observatory, Saint-Petersburg, Russia), BF(Rozhen Observatory, Bulgaria), BG(Astr. Obs. of the Odessa National University, Odessa, Ukraine), BH(Astr. Obs. of the Odessa National University, Odessa, Ukraine), BI(Observatoire de Bordeaux, Floirac, France), BJ(Grupo Astronomico Silos, Zaragoza, Spain; Grup d'Estudis Astronómics, Barcelona, Spain), BK(Institutul Astronomic, Bucuresti, Romania), BL(Sternberg Astronomical Institute, Lomonosov Moscow State University, Russia), BM(GAC, Catania, Italy), BN(Lanester, France), BO(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France), BP(Thorigné, France), BQ(Observatorio S. Zani, Lumezzane, Italy), BR(Elgin, Oregon, USA), BS(Rimavska Sobota, Slovakia), BT(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France), BU(Instituto Politecnico Tomar, Tomar, Portugal), BV(Grupo Astronomico Silos, Zaragoza, Spain; Grup d'Estudis Astronómics, Barcelona, Spain), BW(Ural State University, Ekaterinbourg, Russia), BX(Pulkovo Observatory, Saint-Petersburg, Russia), BY(Institutt for Teorerisk Astrofysikk, Oslo, Norway), BZ(Armagh Observatory, Armagh, Northern Ireland, UK), CA(Crimean Laboratory of the Sternberg Astronomical Institute, Moscow, Russia), CB(Sendai, Japan), CC(Rozhen Observatory, Bulgaria), CD(Pulkovo Observatory, Saint-Petersburg, Russia), CE(Pulkovo Observatory, Saint-Petersburg, Russia), CF(Pulkovo Observatory, Saint-Petersburg, Russia), CG(Observatoire de Bordeaux, Floirac, France), CH(Pulkovo Observatory, Saint-Petersburg, Russia), CI(IIA (Indian Institute of Astrophysics), VBO, Kavalur, India), CJ(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France), CK(Observatoire de Dax, Dax, France), CL(Massa, Italy), CM(Observatoire de Bordeaux, Floirac, France), CN(Observatoire de Paris, Meudon, France), CO(Yunnan Observatory, Kunming, PR China), CP(GAC, Catania, Italy), CQ(Grupo Astronomico Silos, Zaragoza, Spain; Grup d'Estudis Astronómics, Barcelona, Spain), CR(C2AHP, Saint-Michel l'observatoire, France), CS(Czech Astronomical Society, Praha, Czech Rep.), CT(Observatorio S. Zani, Lumezzane, Italy), CU(GAC, Catania, Italy), CV(Armagh Observatory, Armagh, Northern Ireland, UK), CW(Observatorio S. Zani, Lumezzane, Italy), CX(Cluj-Napoca, Romania), CY(C2AHP, Saint-Michel l'observatoire, France), CZ(IIA (Indian Institute of Astrophysics), VBO, Kavalur, India), DA(Mainz, Germany), DB(C2AHP, Saint-Michel l'observatoire, France), DC(Gieres, France), DD(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France; Observatoire de l'université de Lille, Lille, France), DE(Nyrola Observatory, Jyvaskylan, Finland), DF(C2AHP, Saint-Michel l'observatoire, France), DG(Royal Observatory of Belgium, Brussels, Belgium), DH(Jinan University, Guangzhou, PR China), DI(Observatorio S. Zani, Lumezzane, Italy), DJ(Observatory and Planetarium Praha, Czech Rep.), DK(Armagh Observatory, Armagh, Northern Ireland, UK), DL(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France; Observatoire de Bordeaux, Floirac, France), DM(Observatoire de Bordeaux, Floirac, France), DN(Rimavska Sobota, Slovakia), DO(C2AHP, Saint-Michel l'observatoire, France), DP(Thorigné, France), DQ(Universidad de Monterrey, Monterrey, Mexico), DR(GAC, Catania, Italy), DS(C2AHP, Saint-Michel l'observatoire, France), DT(GAC, Catania, Italy), DU(IIA (Indian Institute of Astrophysics), VBO, Kavalur, India), DV(Terskol Observatory, Kabardino-Balkaria, Russia), DW(Pulkovo Observatory, Saint-Petersburg, Russia), DX(Institutul Astronomic, Bucuresti, Romania), DY(Observatorio S. Zani, Lumezzane, Italy), DZ(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France), EA(Sternberg Astronomical Institute, Lomonosov Moscow State University, Russia), EB(Fessenkov Astrophysical Institute, Alma-Ata, Kazakhstan), EC(Institutul Astronomic, Bucuresti, Romania), ED(Cluj-Napoca, Romania), EE(Armagh Observatory, Armagh, Northern Ireland, UK), EF(Pierrevert, France), EG(IIA (Indian Institute of Astrophysics), Bangalore, India), EH(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France), EI(IIA (Indian Institute of Astrophysics), VBO, Kavalur, India), EJ(IIA (Indian Institute of Astrophysics), VBO, Kavalur, India), EK(Grupo Astronomico Silos, Zaragoza, Spain; Grup d'Estudis Astronómics, Barcelona, Spain), EL(Institut de mécanique céleste et de calcul des éphémérides - Observatoire de Paris, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, 75014 Paris, France; Observatoire de l'université de Lille, Lille, France), EM(Mundolsheim, France), EN(Flemish association of amateur astronomers, Groenstraat 12, Mortsel, Belgium), EO(Vienna, Austria)
Publication:
Astronomy and Astrophysics, Volume 493, Issue 3, 2009, pp.1171-1182 (A&A Homepage)
Publication Date:
01/2009
Origin:
EDP Sciences
Astronomy Keywords:
astrometry, eclipses, occultations, planets and satellites: individual: Jupiter
DOI:
10.1051/0004-6361:200810420
Bibliographic Code:
2009A&A...493.1171A

Abstract

Context: In 2003, the Sun and the Earth passed through both the equatorial plane of Jupiter and therefore the orbital planes of its main satellites.
Aims: During this period, mutual eclipses and occultations were observed and we present the data collected.
Methods: Light curves of mutual eclipses and occultations were recorded by the observers of the international campaign PHEMU03 organized by the Institut de mécanique céleste, Paris, France.
Results: We completed 377 observations of 118 mutual events from 42 sites and the corresponding data are presented in this paper. For each observation, information about the telescope, receptor, site, and observational conditions are provided.
Conclusions: This paper gathers all data and indicates a first estimate of its precision. This catalogue of these rare events should constitute an improved basis for accurate astrometric data useful in the development of dynamical models.

Table 4 and lightcurves (in ascii format) are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/493/1171

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