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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
- Information
- Symposium - International Astronomical Union , Volume 37: Non-Solar X- and Gamma-Ray Astronomy , 1970 , pp. 173 - 175
- Copyright
- Copyright © Reidel 1970
References
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
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