International audiencePhoebe is the only major satellite of Saturn with a retrograde orbit. The Cassini Imaging Science Subsystem (ISS) took a lot of Phoebe images between 2004 and 2017, but only a selection of them has been reduced. In this paper, we reduced the remaining ISS images of Phoebe. In the reduction, the Gaia EDR3 catalogue was used to provide the reference stars' positions, and the modified moment was used to measure the centre of image stars and Phoebe. Finally, a total of 834 ISS images of Phoebe have been reduced successfully. Compared with the JPL ephemeris SAT375, Phoebe's positions are consistent. The average residuals in the right ascension and declination are 0.08″ and -0.05'', and the standard deviations of the residua...
Context.The theoretical model of natural satellite motion may need improvement each time new observa...
This work was mainly funded by European Community’s Seventh Framework Program (FP7/2007-2013) under...
Aims. We present astrometric observations of the Saturnian satellites Mimas, Enceladus, Tethys, Dion...
International audiencePhoebe is the only major satellite of Saturn with a retrograde orbit. The Cass...
Context. The Cassini spacecraft has been orbiting Saturn since 2004 and has returned images of satel...
Context. The ephemeris of Phoebe, the ninth satellite of Saturn, is not very accurate. Previous dyna...
In 2003-2004, we obtained 115 new observations of Phoebe, the 9th Saturnian faint satellite (visual ...
Astromeric CCD positions of the Saturnian satellite Phoebe obtained from 60 frames taken in 10 nigh...
International audienceIn order to improve the orbit of Phoebe, the ninth satellite of the Saturnian ...
Astrometric observations of Phoebe, the ninth faint satellite of Saturn with vi-sual magnitude of 16...
Aims. We provide astrometric observations of two of Saturn’s main satellites, Mimas and Enceladus, u...
International audienceAims. We provide astrometric observations of two of Saturn’s main satellites, ...
International audienceIn 1998 and 1999, we started observations of the 9th satellite of Saturn. We m...
Context.The theoretical model of natural satellite motion may need improvement each time new observa...
This work was mainly funded by European Community’s Seventh Framework Program (FP7/2007-2013) under...
Aims. We present astrometric observations of the Saturnian satellites Mimas, Enceladus, Tethys, Dion...
International audiencePhoebe is the only major satellite of Saturn with a retrograde orbit. The Cass...
Context. The Cassini spacecraft has been orbiting Saturn since 2004 and has returned images of satel...
Context. The ephemeris of Phoebe, the ninth satellite of Saturn, is not very accurate. Previous dyna...
In 2003-2004, we obtained 115 new observations of Phoebe, the 9th Saturnian faint satellite (visual ...
Astromeric CCD positions of the Saturnian satellite Phoebe obtained from 60 frames taken in 10 nigh...
International audienceIn order to improve the orbit of Phoebe, the ninth satellite of the Saturnian ...
Astrometric observations of Phoebe, the ninth faint satellite of Saturn with vi-sual magnitude of 16...
Aims. We provide astrometric observations of two of Saturn’s main satellites, Mimas and Enceladus, u...
International audienceAims. We provide astrometric observations of two of Saturn’s main satellites, ...
International audienceIn 1998 and 1999, we started observations of the 9th satellite of Saturn. We m...
Context.The theoretical model of natural satellite motion may need improvement each time new observa...
This work was mainly funded by European Community’s Seventh Framework Program (FP7/2007-2013) under...
Aims. We present astrometric observations of the Saturnian satellites Mimas, Enceladus, Tethys, Dion...