Abstract
Published data from X-ray telescopes are not adequate to reveal the fluctuations in the surface brightness of the background radiation caused by clustering or superclustering of the sources giving rise to the background.
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References
Silk, J., Space Sci. Rev., 11, 671 (1970).
Brecher, K., and Burbidge, G. R., Comments Astrophys. Space Phys., 2, 75 (1970).
Wolfe, A. M., and Burbidge, G. R., Nature, 228, 1170 (1970).
Schwartz, D. A., Boldt, E. A., Holt, S. S., Serlemitsos, P. J., and Bleach, R. D., Nature Physical Science, 233, 110 (1971).
Neymann, J., Scott, E. L., and Shane, C. D., Astrophys. J., 117, 92 (1952).
Brecher, K., Morrison, P., Phys. Rev. Lett., 23, 802 (1969).
Karachentsev, I. D., Astrofizika, 2, 307 (1966).
Scott, E. L., Shane, C. D., and Swanson, M. D., Astrophys. J., 119, 91 (1954).
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WEBSTER, A. Can the Lumpy Distribution of Galaxies be Detected by X-ray observations ?. Nature 238, 20–24 (1972). https://doi.org/10.1038/238020a0
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DOI: https://doi.org/10.1038/238020a0
