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Results from ASCA Sky Surveys
Published online by Cambridge University Press: 25 May 2016
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The origin of the Cosmic X-ray Background (CXB) radiation has been investigated extensively by soft X-ray deep survey imaging observations with Einstein and ROSAT. In contrast, the lack of telescopes capable of detecting hard X-rays has prevented us from extensive study of the nature of the CXB in the energy range above 2 keV before ASCA.
- Type
- Part 5. Extra-Galactic Astronomy
- Information
- Symposium - International Astronomical Union , Volume 179: New Horizons from Multi-Wavelength Sky Surveys , 1998 , pp. 312 - 313
- Copyright
- Copyright © Kluwer 1998
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