Improving source positions in the OCARS catalog: A first approach
Fuente:
arXiv
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| Format: | Preprint |
| Publié: |
2025
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| _version_ | 1866912380641869824 |
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| author | Malkin, Zinovy |
| author_facet | Malkin, Zinovy |
| contents | OCARS (Optical Characteristics of Astrometric Radio Sources) is a compiled catalog of various additional data associated with astrometric radio sources whose coordinates have been determined from very long baseline interferometry (VLBI) observations. It contains source coordinates, object type, redshift, optical and near-infrared magnitudes. Until now, OCARS source coordinates were simply copied from input catalogs and, as a result, were systematically inhomogeneous. This work is the first attempt to obtain a unified set of radio source coordinates aligned to the International Celestial Reference Frame (ICRF), more specically to the third ICRF release, ICRF3. Comparison of the source coordinates in the old OCARS version as of December 2024 and the new OCARS version as of March 2025 with the ICRF3-SX catalog using the vector spherical harmonics (VSH) technique showed almost complete elimination of systematic errors in new OCARS positions relative to the ICRF3 frame. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2505_02805 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Improving source positions in the OCARS catalog: A first approach Malkin, Zinovy Instrumentation and Methods for Astrophysics OCARS (Optical Characteristics of Astrometric Radio Sources) is a compiled catalog of various additional data associated with astrometric radio sources whose coordinates have been determined from very long baseline interferometry (VLBI) observations. It contains source coordinates, object type, redshift, optical and near-infrared magnitudes. Until now, OCARS source coordinates were simply copied from input catalogs and, as a result, were systematically inhomogeneous. This work is the first attempt to obtain a unified set of radio source coordinates aligned to the International Celestial Reference Frame (ICRF), more specically to the third ICRF release, ICRF3. Comparison of the source coordinates in the old OCARS version as of December 2024 and the new OCARS version as of March 2025 with the ICRF3-SX catalog using the vector spherical harmonics (VSH) technique showed almost complete elimination of systematic errors in new OCARS positions relative to the ICRF3 frame. |
| title | Improving source positions in the OCARS catalog: A first approach |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2505.02805 |