CCD Astrometric Observations of Phoebe in 2005-2008

We present relative astrometric measurements of visual binaries made during the second semester of 2005, with the speckle camera PISCO at the 102 cm Zeiss telescope of

The obtained experimental results have demonstrated that relevant time savings can be gained by applying the proposed framework: Not only the effort and expertise required to uses

We compared the observed positions of Mars, Phobos, and Deimos with their theoretical computed positions given by INPOP13c planetary ephemeris (Fienga et al. 2014) and NOE

Figure 1. Combined map of ISS NAC and infrared image taken from VIMS cube “A”. From the inspection of the optical image, it appears that the Phoebe craters are very peculiar,

Moreover, it is important to notice that, in restricted cases, the dynamics of our model overlaps with a simpler dynamical model (see Section 8): this confirms the fact that we

This expression of the back-action function contains the complete description of the atomic state evolution in the weak coupling regime and allows to quantitatively study the

A more restricted way of such interpolation is given by the geometrical multiscale approach, where, based on a domain decomposition, the dimen- sion of the model is adjusted locally

En effet, l’efficacité de la compresse est plus importante en surface qu’en profondeur car elle est de 57% dans le cas d’une application sans pré-mouillage et de 69% pour