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Identification Optique et Photométrie de Radiosources du Catalogue 3CR

Published online by Cambridge University Press:  14 August 2015

Gérard Wlérick
Affiliation:
Observatoire de Paris, Meudon, France
Gérard Lelièvre
Affiliation:
Observatoire de Paris, Meudon, France
Philippe Véron
Affiliation:
Observatoire de Paris, Meudon, France

Abstract

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Using a Lallemand electronic camera, optical identifications for several 3CR radio sources have been made. Photometry has been obtained for objects as faint as B ≃ 21.25. It is suggested that some of the identifications may have redshifts in excess of z = 3.

Type
Research Article
Copyright
Copyright © Reidel 1972 

References

Bibliographie

Adgie, R. L.: 1970, communication personnelle.Google Scholar
Burbidge, G. et Burbidge, M.: 1967, en Quasi-stellar objects, Freeman and Co, San Francisco.CrossRefGoogle Scholar
Elsmore, B. et Mackay, C. D.: 1969, Monthly Notices Roy. Astron. Soc. 146, 360.CrossRefGoogle Scholar
Fomalont, E. B.: 1970, communication personnelle.Google Scholar
Lallemand, A., Canavaggia, R., et Amiot, F.: 1966, Compt. Rend. Acad. Sci. Paris 262, 838.Google Scholar
Sandage, A.: 1970, communication personnelle.Google Scholar
Schmidt, M.: 1968, Astrophys. J. 151, 393.Google Scholar
Walker, M. F. et Kron, G. E.: 1967, Publ. Astron. Soc. Pacific 79, 551.CrossRefGoogle Scholar
Wlérick, G.: 1969, Adv. Electronics Electron Phys. 28B, 787.Google Scholar
Wyndham, J. D.: 1966, Astrophys. J. 144, 459.Google Scholar