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pro vyhledávání: '"J.-E. Arlot"'
Autor:
J.-E. Arlot
Publikováno v:
IAU Symposium
A Giant Step: from Milli-to Micro-arcsecond Astrometry, IAU Symposium 248
A Giant Step: from Milli-to Micro-arcsecond Astrometry, IAU Symposium 248, Oct 2007, Shanghai, China, Nanjing, China. pp.66-73, ⟨10.1017/S1743921308018644⟩
A Giant Step: from Milli-to Micro-arcsecond Astrometry, IAU Symposium 248
A Giant Step: from Milli-to Micro-arcsecond Astrometry, IAU Symposium 248, Oct 2007, Shanghai, China, Nanjing, China. pp.66-73, ⟨10.1017/S1743921308018644⟩
The main goal of the astrometry of solar system objects is to build dynamical models of their motions to understand their evolution, to determine physical parameters and to build accurate ephemerides for the preparation and the exploitation of space
Akademický článek
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Autor:
J. Chapront, G.A. Krasinsky, V.K. Abalakin, J.-E. Arlot, T. Fukushima, M.-F. He, C.Y. Hohenkerk, G.H. Kaplan, H. Kinoshita, J.H. Lieske, H. Schwan, P.K. Seidelmann, M. Standish
Publikováno v:
Transactions of the International Astronomical Union. 25:11-14
Autor:
E. Bowell, G.B. Valsecchi, K. Aksnes, J.-E. Arlot, A. Carusi, J.A. Fernández, A. Lemaître, B.G. Marsden, H. Rickman, V.A. Shor, D.K. Yeomans, J.-X. Zhang
Publikováno v:
Transactions of the International Astronomical Union. 25:187-198
Autor:
E. M. Standish, J. Chapront, V. K. Abalakin, J.-E. Arlot, T. Fukushima, M.-F. He, C. Y. Hohenkerk, G. H. Kaplan, H. Kinoshita, G. A. Krasinsky, J. H. Lieske, H. Schwan, P. K. Seidelmann
Publikováno v:
Transactions of the International Astronomical Union. 24:7-10
The Commission has established its own website (http://ssd.jpl.nasa.gov/iau-comm4/) containing the following main topics: InformationWhere to Obtain EphemeridesRecent Papers and Information Related to EphemeridesObservational Data(Measurements to whi
Autor:
A. Carusi, Hans Rickman, Anne Lemaitre, Brian G. Marsden, J.-E. Arlot, Kaare Aksnes, Donald K. Yeomans, Edward Bowell, Viktor A. Shor, J.-X. Zhang, Giovanni B. Valsecchi
Publikováno v:
Transactions of the International Astronomical Union. 24:140-143
This Comm. 20 triennial report is prepared as a short summary of the scientific progress in the fields of interest, where, by necessity, only a few highlights are to be mentioned. On the Comm. 20 webpage, the interested reader may find a more complet
Autor:
H. J. J. Bulder, J. J. Sacre, C. Ruatti, B. Morando, J. Vidal, J. M. Gomez-Forrellad, F. Sevre, T. Flatres, J. F. Mellilo, J. M. Desbats, A. Piersimoni, J. C. Le Floch, J. Arsenijevic, A. Dipaolantonio, F. Colas, V. Turcu, D. Hube, D. T. Vu, R. Burchi, O. Gherega, Y. Ito, J. Lecacheux, G. de Angelis, H. Takami, G. Oprescu, D. Przewozny, G. de Benedetto, D. Chis, B. Nitschelm, Patrice Bouchet, J. Colin, A. Mallama, Ricard Casas, G. Montignac, W. Thuillot, J. Barroso, V. Shkodrov, G. White, J. F. Le Campion, V. D'Ambrosio, F. Chauvet, M. Rapaport, J. Bourgeois, O. Hainaut, L. Farcas, J. E. Arlot, C. Blanco, C. Bauer, B. Nicolet, J. A. Cano, J. Guarro, A. Horvat, R. Taylor, B. E. Martin, H. Denzau, Mark R. Kidger, J. Souchay, J. Berthier, D. J. Tholen, M. Froeschle, A. Dumitrescu, V. Protitch-Benishek, R. Baptista, M. Federspiel, R. P. Wilds, S. Molau, A. Riou, G. Helmer, P. Descamps, R. Vasundhara, C. Meyer
Publikováno v:
Astronomy and Astrophysics Supplement Series. 125:399-405
In 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
Publikováno v:
Icarus. 125:465-470
The space probe Voyager discovered an intense volcanism on Io, the first Galilean satellite of Jupiter, in 1979. The series of Io's occultations by the other Galilean satellites occurring in 1997–1998 presents an excellent opportunity to observe th
Autor:
François Colas, J. E. Arlot
Publikováno v:
CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY. 66:123-130
Astrometry in the solar system made more progress during the past ten years than it did during the seven or eight decades before. In fact, the development of large refractors with micrometers, and after the improvement of the photographic technique,