Corrected proper motion for HIP stars Virtual Observatory Resource

Authors
  1. Damljanovic G.
  2. Milic I.S.
  3. Published by
    CDS
Abstract

During the last century, there were many so-called independent latitude (IL) stations with the observations which were included into data of a few international organizations (like Bureau International de l'Heure - BIH, International Polar Motion Service - IPMS) and the Earth rotation programmes for determining the Earth Orientation Parameters - EOP. Because of this, nowadays, there are numerous astrometric ground-based observations (made over many decades) of some stars included in the Hipparcos Catalogue (ESA 1997, Cat. I/239). We used these latitude data for the inverse investigations - to improve the proper motions in declination {mu}_{delta}_ of the mentioned Hipparcos stars. We determined the corrections {Delta}{mu}_{delta}_ and investigated agreement of our {mu}_{delta}_ and those from the catalogues Hipparcos and new Hipparcos (van Leeuwen 2007, Cat. I/311). To do this we used the latitude variations of 7 stations (Belgrade, Blagoveschtschensk, Irkutsk, Poltava, Pulkovo, Warsaw and Mizusawa), covering different intervals in the period 1904.7-1992.0, obtained with 6 visual and 1 floating zenith telescopes (Mizusawa). On the other hand, with regard that about two decades have elapsed since the Hipparcos ESA mission observations (the epoch of Hipparcos catalogue is 1991.25), the error of apparent places of Hipparcos stars has increased by nearly 20mas because of proper motion errors. Also, the mission lasted less than four years which was not enough for a sufficient accuracy of proper motions of some stars (such as double or multiple ones). Our method of calculation, and the calculated {mu}_{delta}_ for the common IL/Hipparcos stars are presented here. We constructed an IL catalogue of 1200 stars: there are 707 stars in the first part (with at least 20 years of IL observations) and 493 stars in the second one (less than 20 years). In the case of {mu}_{delta}_ of IL stars observed at some stations (Blagoveschtschensk, Irkutsk, Mizusawa, Poltava and Pulkovo) we find the formal errors less than the corresponding Hipparcos ones and for some of them (stations Blagoveschtschensk and Irkutsk) even less than the new Hipparcos ones.

Keywords
  1. Astrometry
  2. Proper motions
Bibliographic source Bibcode
2011SerAJ.182...35D
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/Ser/182.35
IVOA Identifier IVOID
ivo://CDS.VizieR/J/other/Ser/182.35

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/Ser/182.35
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/Ser/182.35
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/other/Ser/182.35
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/other/Ser/182.35/table2?
https://vizier.iucaa.in/viz-bin/conesearch/J/other/Ser/182.35/table2?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/other/Ser/182.35/table2?

History

2012-01-05T15:05:56Z
Resource record created
2012-01-05T15:05:56Z
Created
2017-10-03T05:12:34Z
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