All Tables

Table 1: Input catalogues. The last column shows number of sources in the catalogue and the number of reference sources used to tie the orientation of the catalogue to the ICRF.
Table 2: WRMS differences between the input catalogues and the ICRF before (Raw) and after approximation of the systematic differences (see notation of the methods in text). Results related to the LF method, providing the best approximation, are shown in bold. Unit: $\mu$ as.
Table 3: Weights of the input catalogues applied during combination, averaged over the sky.
Table 4: WRMS differences between the input catalogues and the combined catalogue RSC(PUL)07C02. Unit: $\mu$ as.
Table 5: Scatter of the celestial pole offset time series obtained with two catalogues. The FCN column shows the scatter with respect to the FCN model, the WADEV column shows the weighted Allan deviation. Unit: $\mu$ as.