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| Name：Victorludge | 21, Nov, 2023 11:16:34 | |
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the observed deficiencies in the APM survey area and for [b] >20 represent 2.5 and 4.0 fluctuations in the local galaxy distribution respectively. These results are therefore potentially at odds with the form of clustering expected on large scales. We examine the form of galaxy clustering to 1 sc | |
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