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Densification of the Optical Reference Frame (Commission 8) |
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Objectives and HistoryThis group works towards obtaining high precision astrometry of optical sources and putting those on the system of the ICRS. This is being undertaken for the express purpose of increasing the density (number of stars per square degree) beyond that of the Hipparcos Catalogue, which defines the optical reference frame. The Densification of the Optical Reference
Frame sub-group originated
under the International Celestial Reference System (ICRS) Working Group
sponsored by Division I of the International Astronomical Union. At the 2003 IAU
General
Assembly, the ICRS Working Group was essentially dissolved. The
Densification
of the Optical Reference Frame group was moved under
Commission 8.
At the 2006 GA in Prague this WG was confirmed to continue for the
2006-2009 period. At left are links relevant to the
Densification sub-group, including a summary of the current status of Optical Astrometric Surveys. The following is another useful resource,
summarizing astrometric surveys
past,
present and future. |
last update: 2009 July 06