Zobrazeno 1 - 10
of 40
pro vyhledávání: '"G. Dourneau"'
Autor:
K. X. Shen, X. Cheng, H. Y. Zhang, S. H. Wang, G. Dourneau, Dahai Yan, Shanshan Li, X. J. Xi, D. Harper, R. C. Qiao
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2014, 438 (2), pp.1663-1668. ⟨10.1093/MNRAS/STT2304⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2014, 438 (2), pp.1663-1668. ⟨10.1093/MNRAS/STT2304⟩
International audience; In this paper, we used the 3108 Earth-based astrometric observations from the Natural Satellite Data Center over more than 30 yr time span from 1975 to 2006 for determining the epoch state vectors of the Neptunian largest sate
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 457, pp.2900-2907. ⟨10.1093/mnras/stw120⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 457, pp.2900-2907. ⟨10.1093/mnras/stw120⟩
International audience; Old astrophotographic plates are precious sources of historical data for astronomical studies, especially regarding the improvement of natural satellite orbits. Today, with the advent of new, accurate techniques, these old dat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b79ff701d19cf48c78f89ad8577fd530
http://hdl.handle.net/20.500.12278/95858
http://hdl.handle.net/20.500.12278/95858
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 417:2387-2391
In recent years, many new CCD observations of Phoebe, the ninth Saturnian satellite, were published. In this paper, we have used all the observations of Phoebe available until 2009 to update Phoebe's orbit. These observations represent a total number
Autor:
X. Cheng, X. J. Xi, H. Y. Zhang, Z. X. Qi, R. C. Qiao, S. H. Wang, G. Dourneau, K. X. Shen, Zheng-Hong Tang
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 413:1079-1082
Astrometric observations of Phoebe, the faint ninth satellite of Saturn, with a visual magnitude of 16.5, were performed during four successive oppositions in 2005, 2006, 2007 and 2008. A total of 1173 new observed positions of Phoebe, representing m
Autor:
X. Cheng, K. X. Shen, X. Y. Hu, X. J. Xi, Zheng-Hong Tang, R. C. Qiao, S. H. Wang, G. Dourneau
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 391:1791-1795
In this paper, we present 112 new CCD astrometric positions of Nereid, the second and faint satellite of Neptune (mv � 19). We observed this small satellite in the 2006–2007 period with the 1 and 2.16-m telescopes of Xinglong Station near Beijing
Autor:
M. I. Varfolomeev, Nello Ruocco, J. Prost, J. Garlitz, Brian Loader, A. Amossé, J. Mcfarland, C. Druon, Christian Napoli, J. Grismore, A. Sonka, M. Unwin, D. N. da Silva Neto, C. Lopresti, Alexios Liakos, J. Rovira, S. Degenhardt, G. Estraviz, S. Combe, A. Douvris, R. Vieira-Martins, G. Dourneau, J. F. Le Campion, A. Dias-Oliveira, Marcelo Assafin, E. Tontodonati, F. Bragas-Ribas, N. I. Koshkin, Zheng-Hong Tang, Shaolin Li, H. Pavlov, Benoît Noyelles, Andrea Marchini, T. Pauwels, L. Shakun, G. Sbarufatti, F. Colas, Brad Timerson, R. Maulella, J. Vilar, S. Yu. Gorda, M. Ishida, M. Delcroix, K. Miyashita, M. Constantinescu, D. F. Guo, Gennaro Marino, V. Priban, C. K. Ellington, R. Venable, K. Tigani, Gianluca Masi, C. Perelló, D. Gault, E. Lo Savio, Shilong Liao, V. G. Tejfel, M. Ida, A. Collard, R. Zambelli, F. Casarramona, T. George, J. P. Rousselle, P. Farissier, Fabio Salvaggio, L. Barbieri, C. Arena, S. Bolzoni, A. Scheck, G. Dangl, D. Herald, John Talbot, B. Klemt, Jean-Eudes Arlot, William Thuillot, Q. Y. Peng, Ricard Casas, R. Ruisi, P. De Cat, N. V. Sinyaeva, V. Tsamis, A. V. Ivanov, P. Vingerhoets, C. Sciuto, H. Watanabe, H. X. Yin, A. Farmakopoulos, Yong Yu, Apostolos A. Christou, Julio Camargo, A. Sofia, S. Razemon, N. V. Emelyanov, A. Massalle
Publikováno v:
Astronomy and Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2014, 572, pp.A120. ⟨10.1051/0004-6361/201423854⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2014, 572, pp.A120. 〈10.1051/0004-6361/201423854〉
Astronomy and Astrophysics-A&A, EDP Sciences, 2014, 572, pp.A120. ⟨10.1051/0004-6361/201423854⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2014, 572, pp.A120. ⟨10.1051/0004-6361/201423854⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2014, 572, pp.A120. 〈10.1051/0004-6361/201423854〉
Astronomy and Astrophysics-A&A, EDP Sciences, 2014, 572, pp.A120. ⟨10.1051/0004-6361/201423854⟩
Context. In 2009, the Sun and the Earth passed through the equatorial plane of Jupiter and therefore the orbital planes of its main satellites. It was the equinox on Jupiter. This occurrence made mutual occultations and eclipses between the satellite
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8501a42d8f0db832883ca0c11b38f3e5
http://hdl.handle.net/20.500.12278/96031
http://hdl.handle.net/20.500.12278/96031
Publikováno v:
Astronomy & Astrophysics. 367:1061-1069
This paper presents an analysis of astrometric reduction methods for the calibration of a CCD target. To compare these methods, we collected about 3000 recent CCD observations between 1990-1997. We discuss the comparison of the four main contemporary
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2013, 428 (3), pp.2755-2764. ⟨10.1093/mnras/sts240⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2013, 428 (3), pp.2755-2764. ⟨10.1093/mnras/sts240⟩
International audience; An observational campaign of the five Uranian major satellites was carried out during the period 1998-2007. A total of 2358 satellite observations in 1025 CCD frames were taken at two observational stations near Beijing and Sh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0fe6f8044c4c9bc4bdc4baf01d78ea74
https://hal.archives-ouvertes.fr/hal-00763960
https://hal.archives-ouvertes.fr/hal-00763960
Autor:
D. L. Gorshanov, O. Dechambre, Ricard Casas, A. Sergeev, A. Murphy, Brian Loader, G. Dourneau, F. Colas, A. Kurenya, A. Farmakopoulos, Marcelo Assafin, V. Kozlov, Julio Camargo, J. F. Le Campion, A. Dias-Oliveira, P. Valdes Sada, D. N. da Silva Neto, V. Tsamis, X. Zhang, D. Gault, J. Lecacheux, N. V. Emelyanov, Dave Herald, Apostolos A. Christou, Felipe Braga-Ribas, A. Massalle, R. Vieira-Martins, Jean-Eudes Arlot, T. George, N. Parakhin, Maksim V. Andreev, C. Schnabel, Valery Lainey, Alexandre Roman-Lopes, M. Mc Brien
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2012, 544, pp.29. ⟨10.1051/0004-6361/201118509⟩
Astronomy and Astrophysics-A&A, 2012, 544, pp.29. ⟨10.1051/0004-6361/201118509⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2012, 544, pp.29. ⟨10.1051/0004-6361/201118509⟩
Astronomy and Astrophysics-A&A, 2012, 544, pp.29. ⟨10.1051/0004-6361/201118509⟩
Context. The photometry of mutual occultations and eclipses of natural planetary satellites can be used to infer very accurate astrometric data. This can be achieved by processing the light curves of the satellites observed during international campa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3a283a9846bc49e682b3e3685fa13ccd
http://hdl.handle.net/20.500.12278/96667
http://hdl.handle.net/20.500.12278/96667
Autor:
G. Dourneau, Kaare Aksnes
Publikováno v:
Icarus. 112:545-548
Around the times of the passages of Earth and the Sun through Saturn's ringplane, 198 mutual occultations and eclipses are predicted to occur between Saturn's major satellites between January 1995 and December 1996. To aid photometric observations, p