OGLE3 Magellanic Clouds High proper motion stars Virtual Observatory Resource

Authors
  1. Poleski R.
  2. Soszynski I.
  3. Udalski A.
  4. Szymanski M.K.
  5. Kubiak M.,Pietrzynski G.
  6. Wyrzykowski L.
  7. Ulaczyk K.
  8. Published by
    CDS
Abstract

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.

Keywords
  1. magellanic-clouds
  2. proper-motions
Bibliographic source Bibcode
2011AcA....61..199P
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AcA/61/199
IVOA Identifier IVOID
ivo://CDS.VizieR/J/AcA/61/199

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AcA/61/199
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AcA/61/199
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AcA/61/199
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/AcA/61/199/ident?
https://vizier.iucaa.in/viz-bin/conesearch/J/AcA/61/199/ident?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AcA/61/199/ident?

History

2011-11-29T08:53:31Z
Resource record created
2011-11-29T08:53:31Z
Created
2017-09-20T05:13:52Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr