The number of known Near-Earth Objects (NEOs) has rapidly increased in rece
nt years. The discovery effort must be succeeded by follow-up observations
to ensure astrometric data for determining orbits of newly discovered NEOs.
The importance of follow-up astrometry of NEOs increases with the rising n
umber of discovered NEOs. The field of follow-up astrometry includes the co
nfirmatory observations, early and later follow-up observations, as well as
the recoveries of NEOs in the second convenient opposition. We discuss her
e methods, techniques and results of the targeted NEO follow-up astrometry
programme at the Klet' Observatory using the 0.57 m telescope, equipped wit
h a CCD camera since 1994. We point out that follow-up astrometry of NEOs i
s the common endeavour of the whole international community; this is also b
ased on the continued improvement of communication tools. In the near futur
e we are going to extend this programme to fainter objects and very fast-mo
ving objects using a 1.02 m reflector at Klet'. (C) 2000 Elsevier Science L
td. All rights reserved.