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Investigations on Optical and Radio Reference Frames

Published online by Cambridge University Press:  12 April 2016

S. Puliaev  and
A.H. Andrei
S. Puliaev*
Affiliation:
Observatório Nacional Rio de Janeiro - RJ, Brazil
A.H. Andrei
Affiliation:
Observatório Nacional Rio de Janeiro - RJ, Brazil
*
1On leave from Pulkovo Observatory, St. Petersburg, Russia

Abstract

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Features of the systematic errors of the Carlsberg Automatic Meridian Circle (CAMC) reference frame are investigated using a secondary radio reference frame defined by a set of astrometric VLA, VLBI and submillimetric positions of radio stars, taken from the literature. The radio positions of 62 stars are compared against the corresponding CAMC positions. The systematic errors of the CAMC catalogue are found to be generally smaller than 005. The radio positions were also compared with the positions obtained with the Bordeaux Automatic Meridian Circle (BORD). It was found a good coincidence between (CAMC–Radio) and (BORD–Radio) systematic differences.

Type
Reference Systems and Astronomical Standards
Information
International Astronomical Union Colloquium , Volume 165: Dynamics and Astrometry of Natural and Artificial Celestial Bodies , 1997 , pp. 449 - 452
Copyright
Copyright © Kluwer 1997

References

Andrei, A.H., Jilinski, E.G., and Puliaev, S.P.: 1995, Astron. J. 109, 428–433.Google Scholar
Assafin, M., Vieira-Martins, R., and Andrei, A.H.: 1996, this volume.Google Scholar
Baudry, A., Lucas, R., and Guilloteau, S.: 1995, Astron. Astrophys. 293, 594–604.Google Scholar
Bowers, P.F., Johnston, K.J., and Spencer, J.H.: 1983, Astrophys. J. 274, 733.Google Scholar
Carlsberg Meridian Catalogues No 1-4, 5, 6, 7, 8: 1990, 1991, 1992, 1993, 1994, Copenhagen University Observatory, Royal Greenwich Observatory and Real Instituto y Observatório de la Armada en San Fernando.Google Scholar
de Vegt, C. and Gehlich, U.K.: 1982, Astron. Astrophys. 113, 213.Google Scholar
Johnston, K.J., de Vegt, C., Florkowski, D.R., and Wade, C.M.: 1985, Astron. J. 90, 2381.Google Scholar
Lestrade, J.-F., Jones, D.L., Preston, R.A., Phillips, R.B., Titus, M.A., Kovalevsky, J., Lin-degren, L., Hering, R., Froeshlé, M., Falin, J.-L., Mignard, F., Jacobs, C.S., Sovers, O.J., Eubanks, M., and Gabuzda, D.: 1995, Astron. Astrophys. 304, 182–188.Google Scholar
Lindegren, L., Roser, S., Schrijver, H., Lattami, M.G., van Leeuwen, F., Perryman, M.A.C., Bernacca, P.L., Falin, J.L., Froeshlé, M., Kovalevsky, J., Lenhardt, H., and Mignard, F.: 1995, Astron. Astrophys. 304, 44–51.Google Scholar
Morrison, L.V., Argyle, R.W., Requieme, Y., and Mazurier, J.M.: 1990, Astron. Astrophys. 236, 256–260.Google Scholar
Requieme, Y. and Mazurier, J.M.: 1991, Astron. Astrophys. 89, 311–318.Google Scholar
Stone, R.C.: 1994, Astron. J. 108, 313–325.CrossRefGoogle Scholar