Pd. Hemenway et al., THE PROGRAM TO LINK THE HIPPARCOS REFERENCE FRAME TO AN EXTRAGALACTICREFERENCE SYSTEM USING THE FINE GUIDANCE SENSORS OF THE HUBBLE-SPACE-TELESCOPE, The Astronomical journal, 114(6), 1997, pp. 2796-2810
The Hipparcos Satellite Mission has produced positions, proper motions
, and parallaxes of unprecedented accuracy for 118,000 stars. For the
positions and proper motions to represent true directions and physical
motions in space, they must refer to an accurate realization of a non
rotating (inertial) reference frame. One of the major problems confron
ting the Hipparcos Project was the determination of the relationship o
f the satellite coordinate system to the best available celestial coor
dinate system, hopefully at an accuracy approaching the systematic acc
uracy of the Hipparcos satellite itself. In 1978 we recognized the pos
sibility of using the Fine Guidance Sensors of the Hubble Space Telesc
ope (HST) to measure the Hipparcos coordinate offset and its time vari
ation with respect to extragalactic objects, and we undertook that pro
ject. The first HST observation for the project was made in 1993 April
, and the last observation used in the solution was made in 1995 Octob
er. The HST data consist of accurate angular separations of Extragalac
tic Objects from Hipparcos stars. Ultimately the HST solution was inco
rporated with other techniques to form the final link between Hipparco
s and the International Celestial Reference System. This link determin
ed the final catalogue system for the published Hipparcos data. We des
cribe the problem, the instrumentation of the two space missions, the
limitations imposed by the missions on the observations, the reduction
and analysis procedures, and the final results with respect to the fi
nal Hipparcos solution. We determine the relation of the Hipparcos coo
rdinate axes with respect to the ICRS coordinate axes from the HST, Hi
pparcos, and VLBI data alone. The rms uncertainties are about 2 millia
rcseconds for the angular offsets and about 2.5 milliarcseconds/yr for
the angular rotations. (C) 1997 American Astronomical Society. [S0004
-6256(97)03612-1].