Corrections between UCAC3 and PPMXL

Differences between UCAC3 and PPMXL in positions and proper motions, on an all-sky one-degree grid. At each gridpoint we give the differences X(PPMXL)- X(UCAC3) averaged over all stars in a sqrt(2)/2-degrees environment around the gridpoint given. The corrections given here should bring UCAC3 based astrometry to the ICRS.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/org.gavo.dc/ucac3/q/corr
Related Identifier http://dc.zah.uni-heidelberg.de/ucac3/q/corr/info
Related Identifier http://dc.zah.uni-heidelberg.de/ucac3/q/corr/form
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://org.gavo.dc/ucac3/q/corr
Provenance
Creator GAVO Data Center
Publisher The GAVO DC team
Publication Year 2009
OpenAccess true
Contact GAVO Data Center Team <gavo(at)ari.uni-heidelberg.de>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics