I observed, with my friend Costantino Sigismondi and his students, the occultation of BY Cancri by Saturn and its rings on 2006 January 25. This star is a delta Scuti variable with a very small amplitude, is catalogued as HIP 42705 or SAO 98054 and its brightness is 7.91-7.92 mag. This star belongs to M44, also called Praesepe cluster (Latin for “manger”).
I have shot some picture of Saturn like this:

thanks of Costantino’s reflector telescope and realized with a time exposure of 1/10 seconds at 400 ISO and f/4.9.
Later, with a longer time exposure (1 second at 400 ISO and f/2,8), I’ve captured the image of 3 Saturn’s satellites and of 2 star of the Praesepe cluster, including BY Cancri, labelled with its SAO number, barely visible out of Saturn disk:

Of course the elongated shape of Saturn and the line-like stars are due to the Earth rotation and, consequently, to the rotation of the celestial sphere.
For further infomation on this occultation, I suggest to visite the IOTA page on this event.