OGLE3 Magellanic Clouds High proper motion stars

We present the results of a search for High Proper Motion (HPM) stars, i.e., the ones with pm>100mas/yr, in the direction to the Magellanic Clouds. This sky area was not examined in detail as the high stellar density hampers efforts in performing high-quality astrometry.

Cone search capability for table J/AcA/61/199/ident (Main catalog file)

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/AcA/61/199
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AcA/61/199
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AcA/61/199
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/AcA/61/199
Provenance
Creator Poleski R.; Soszynski I.; Udalski A.; Szymanski M.K.; Kubiak M.,Pietrzynski G.; Wyrzykowski L.; Ulaczyk K.
Publisher CDS
Publication Year 2011
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Physics