http://arxiv.org/abs/2105.11296
Despite continuous increasing of the number of ICRF sources, their sky coverage is still not satisfactory. The goal of this study is to discuss some new considerations for extending the ICRF source list. Statistical analysis of the ICRF catalog allows us to identify less populated sky regions where new ICRF sources or additional observations of the current ICRF sources are most desirable to improve both the uniformity of the source distribution and the uniformity of the distribution of the position errors. It is also desirable to include more sources with high redshift in the ICRF list. These sources may be of interest for astrophysics. To select prospective new ICRF sources, the OCARS catalog is used. The number of sources in OCARS is about three times greater than in the ICRF3, which gives us an opportunity to select new ICRF sources that have already be tested and detected in astrometric and geodetic VLBI experiments.
Z. Malkin
Tue, 25 May 21
56/75
Comments: Presented at the 25th Working Meeting of the European VLBI Group for Geodesy and Astrometry (EVGA), 15-18 March 2021 (virtual). Submitted to the Conference Proceedings. arXiv admin note: text overlap with arXiv:1808.10035
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