Abstract
The Seventh Orbiting Solar Observatory, OSO-7, carries on board a 1–60 keV X-ray detector for the purpose of measuring the positions, spectra and time variations of X-ray sources. The instrument is described herein, and several topics under investigation and results in publication are mentioned.
Supported in part by Contract NGL 22-009-115 from the National Aeronautics and Space Administration.
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Clark, G. W., Bradt, H. V., Lewin, W. H. G., Markert, T. H., Schnopper, H. W., and Sprott, G. F.: 1972a, Astrophys. J.,in press.
Clark, G. W., Bradt, H. V., Lewin, W. H. G., Markert, T. H., Schnopper, H. W., and Sprott, G. F.: 1972b, Astrophys. J. Letters,in press.
Doxsey, R., Murthy, G. T., Rappaport, S., Zaumen, W., and Spencer, J.: 1972, Astrophys. J. Letters 176, L15.
Liller, W.: 1972, IAU Circular 2415 and 2427.
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© 1973 International Astronomical Union
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Clark, G.W. (1973). Observations of Cosmic X-ray Sources by the MIT Instrument on the OSO-7. In: Bradt, H., Giacconi, R. (eds) X- and Gamma-Ray Astronomy. International Astronomical Union/Union Astronomique Internationale, vol 55. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2585-0_3
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DOI: https://doi.org/10.1007/978-94-010-2585-0_3
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