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Identification of X-ray sources at Cerro Tololo inter-American observatory

Published online by Cambridge University Press:  14 August 2015

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The telescope used for identification of X-ray sources at the Cerro Tololo Inter-American Observatory is the Curtis Schmidt Telescope. This telescope is located at Tololo by agreement with the University of Michigan. The field of the telescope is 5° × 5° and its correcting aspheric plate has negligible chromatic aberration over the range 3200 to 10000 Å. This latter feature makes it an ideal instrument for multicolor survey work.

Type
Research Article
Copyright
Copyright © Reidel 1970 

References

Blanco, V. M.: 1967, I.A.U. Circular No. 2035.Google Scholar
Blanco, V. M., Kunkel, W. E., and Hiltner, W. A.: 1968, Astrophys. J. 152, L137. See also Freeman, K. C., Rodgers, A. W., and Lyngå, G.: 1968, Nature 219, 251.CrossRefGoogle Scholar
Eggen, O. J. and Lyngå, G.: 1968, Astrophys. J. 153, L195.CrossRefGoogle Scholar
Feast, M. W.: 1967, Nature 215, 1158.CrossRefGoogle Scholar
Gursky, H., Kellogg, E. M., and Gorenstein, P.: 1968, Astrophys. J. 154, L71.CrossRefGoogle Scholar