Improving the S/X Celestial Reference Frame in the South: A Status Update
SCHARTNER, M
Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] [ETH Zürich]
< Leer menos
Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] [ETH Zürich]
Idioma
en
Communication dans un congrès
Este ítem está publicado en
25th Working Meeting of the European VLBI Group for Geodesy and Astrometry (EVGA), 2021-03-15, Cyberspace.
Resumen en inglés
Catalogs of positions of compact extragalactic radio sources, including the ICRF-3, are generally weaker in the south by factors of 2 or more in both density and precision. In 2018 we started a campaign to improve the S/X ...Leer más >
Catalogs of positions of compact extragalactic radio sources, including the ICRF-3, are generally weaker in the south by factors of 2 or more in both density and precision. In 2018 we started a campaign to improve the S/X celestial reference frame in the South by upgrading existing IVS astrometric observing programmes. Our efforts were mainly focused on the Celestial Reference Frame (CRF) and Celestial Reference Frame Deep South (CRDS) sessions, which are dedicated astrometric observing programmes of sources at mid-and southern declinations. In particular, the data rate of the CRF and CRDS< Leer menos
Palabras clave en inglés
Astrometry
VLBI
Celestial Reference Frame
Southern Hemisphere
quasars
Orígen
Importado de HalCentros de investigación