Guardado en:
| Autores principales: | , , , , , , , , , , , , |
|---|---|
| Formato: | Preprint |
| Publicado: |
2026
|
| Materias: | |
| Acceso en línea: | https://arxiv.org/abs/2605.27629 |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
| _version_ | 1866914606615625728 |
|---|---|
| author | Gordon, David de Witt, Aletha Jacobs, Christopher S. Krasna, Hana Bertarini, Alessandra McCallum, Jamie Quick, Jonathan Garcia-Miro, Cristina Jung, Taehyun Hodgson, Jeffrey A. Cheong, Whee Yeon Lee, Sang-Sung Byun, Do-Young |
| author_facet | Gordon, David de Witt, Aletha Jacobs, Christopher S. Krasna, Hana Bertarini, Alessandra McCallum, Jamie Quick, Jonathan Garcia-Miro, Cristina Jung, Taehyun Hodgson, Jeffrey A. Cheong, Whee Yeon Lee, Sang-Sung Byun, Do-Young |
| contents | We present an updated K band (24 GHz) celestial reference frame (CRF) constructed from 3.5 million Very Long Baseline Interferometry (VLBI) observations collected during 211 observing epochs between May 2002 and December 2025 using the Very Long Baseline Array (VLBA), the HARTRAO-HOBART26 baseline, the HARTRAO-YEBES40M baseline, and the Korean VLBI Network (KVN) augmented with several other VLBI stations. We have successfully observed and determined precise angular coordinates for 1317 compact extragalactic radio sources, essentially quasars, covering the full sky. This updated K band catalog is designated as CRF-K-2025. The precision of CRF-K-2025 is characterized by median scaled uncertainties of 60 and 104 micro-arc-seconds in right ascension and declination, respectively. The increase in number of observations and sensitivity over earlier K band campaigns has resulted in a catalog with 493 additional sources and a precision approximately 25% better than the ICRF3-K catalog, and similar to the ICRF3-SX catalog. At K band, these quasar radio sources generally show less extended emission than at lower frequencies and thus can potentially provide a more stable long term celestial reference frame than at the standard S/X (2.3/8.4 GHz) observing bands of ICRF3-SX. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2605_27629 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | The Celestial Reference Frame at K Band: The CRF-K-2025 Catalog Gordon, David de Witt, Aletha Jacobs, Christopher S. Krasna, Hana Bertarini, Alessandra McCallum, Jamie Quick, Jonathan Garcia-Miro, Cristina Jung, Taehyun Hodgson, Jeffrey A. Cheong, Whee Yeon Lee, Sang-Sung Byun, Do-Young Astrophysics of Galaxies We present an updated K band (24 GHz) celestial reference frame (CRF) constructed from 3.5 million Very Long Baseline Interferometry (VLBI) observations collected during 211 observing epochs between May 2002 and December 2025 using the Very Long Baseline Array (VLBA), the HARTRAO-HOBART26 baseline, the HARTRAO-YEBES40M baseline, and the Korean VLBI Network (KVN) augmented with several other VLBI stations. We have successfully observed and determined precise angular coordinates for 1317 compact extragalactic radio sources, essentially quasars, covering the full sky. This updated K band catalog is designated as CRF-K-2025. The precision of CRF-K-2025 is characterized by median scaled uncertainties of 60 and 104 micro-arc-seconds in right ascension and declination, respectively. The increase in number of observations and sensitivity over earlier K band campaigns has resulted in a catalog with 493 additional sources and a precision approximately 25% better than the ICRF3-K catalog, and similar to the ICRF3-SX catalog. At K band, these quasar radio sources generally show less extended emission than at lower frequencies and thus can potentially provide a more stable long term celestial reference frame than at the standard S/X (2.3/8.4 GHz) observing bands of ICRF3-SX. |
| title | The Celestial Reference Frame at K Band: The CRF-K-2025 Catalog |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2605.27629 |