Poster presented at the International Conference of the Astronomische Gesellschaft ,
Göttingen, 20.-25. September 1999
Abstract published in : Astronomische Gesellschaft Abstract Series 15  ,  145

Search for unmodelled effects in Hipparcos abscissa residuals

H.Lenhardt, R.Hering and H.G.Walter
Astronomisches Rechen-Institut, Mönchhofstrasse 12 -14, D-69120 Heidelberg, Germany

 

The abscissa residuals provided by the FAST and NDAC data reduction consortia are published in the Hipparcos Catalogue (ESA 1997). Applying single star criteria and a goodness-of-fit parameter |F2| smaller than 1.0 we selected 1 944 098 and 2 002 496 residuals corresponding to 63 216 FAST and 62 984 NDAC stars, respectively. These residuals serve formally as `observations' in a weighted least-squares adjustment . Proceeding from Murray (1981) we investigate the existence of : (1), a deviation  from the value = 1 assumed in the General Theory of Relativity, (2), a zero-point correction of the Hipparcos parallaxes and, (3), linear and quadratic variations with time.
 
A correlation exceeding 0.9 was found between and the zero-point correction, which suggests the avoidance of simultaneous estimations of these parameters. In these circumstances we obtain = 0.0027 ± 0.0014  from the FAST residuals, while the NDAC residuals yield the insignificant value = -0.0010 ± 0.0016  probably due to the fact that the final NDAC sphere solution had already taken account of the - parameter. For both sets of residuals the zero-point corrections are negligibly small and statistically insignificant. The linearly time-dependent term is of the order of 0.02 milliarcsecond/yr in FAST and NDAC, but of opposite sign. Their 10-  and 7- significance is remarkable. Moreover, a significant quadratic time dependence results from the FAST residuals.
more about
 data used

 

References

ESA , 1997, The Hipparcos and Tycho Catalogues, ESA SP-1200
Murray,C.A., 1981, Mon.Not.R.astr.Soc. 195, 639


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Created: 13 Jul 1999

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