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Optical Positions for a Sample of ICRF Sources

机译:ICRF源样品的光学位置

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The aim of this paper is to present a large, coherent set of astrometric optical positions for ICRF sources in the Hipparcos reference frame. For this, we present positions for 315 ICRF sources measured in Digitized Sky Survey (DSS) images, with positions referred to the ACT, Hipparcos, and Tycho catalogs. The reductions were made relative to Hubble Space Telescope guide stars, which were previously corrected toward those same catalogs. The reductions errors are at 45 mas and even smaller for southern sources. The comparison between optical with ICRF radio positions shows that neither the residuals nor the internal errors exhibit any trend with magnitudes or with location on the DSS plates.
机译:本文的目的是为Hipparcos参考系中的ICRF源提供一组大而连贯的天文光学位置。为此,我们展示了在数字化天空测量(DSS)图像中测得的315个ICRF源的位置,这些位置参考了ACT,Hipparcos和Tycho目录。相对于哈勃太空望远镜的指南星进行了减少,之前已对那些相同的目录进行过校正。减少误差为45 mas,对于南方来源,误差更小。光学位置与ICRF无线电位置之间的比较表明,残差和内部误差都不会随幅度或位置在DSS板上显示任何趋势。

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