We nd that the observed log Nlog S relation of X-ray clusters can be reproduced remarkably well with a certain range of values for the uctuation amplitude and the cosmological density parameter p 8 in cold dark matter (CDM) universes. The 1 p condence limits on in the CDM models with ) 0 p 8 n \ 1 and h \ 0.7 are expressed as and (0.54
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Kitayama et al. (1997) studied this question.
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