Abstract
AbstractThe reliable orbit determination of newly discovered NEOs is impossible without precise follow-up astrometry in a sufficient arc of observations. This paper describes the follow-up astrometry NEO programme at the Kleť Observatory. Since 1994 we have used a 0.57-m reflector equipped with CCD camera for confirmations of newly discovered NEO candidates, early follow-up astrometry of NEOs in discovery opposition, recovery of NEOs in second opposition and also follow-up astrometry of poorly observed NEOs in further oppositions. In this field the Kleť Observatory is one of the most productive sites in the world. This programme will be extended to fainter objects with the new 1.02-m reflector − which will become operational at the end of 1998.
Published Version
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