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- W1984652555 abstract "We present our first results on large-scale structure in the Universe from a uniform survey of ≳ 2 million galaxies brighter than bJ = 20.5 constructed from machine scans of 185 UK Schmidt plates. We show that over a range of three magnitudes the galaxy two-point angular correlation function, w(θ), scales with depth as expected if we are measuring real clustering in the galaxy distribution. Our correlation functions show a break from a power law at roughly the same physical separation as found by Groth & Peebles from their analysis of the Lick catalogue, but our measurements decline much more gently from a power law on larger scales. We argue that Groth & Peebles may have removed some intrinsic clustering when they corrected for large-scale gradients in the Lick counts. Our analysis has important implications for theories of the formation of large-scale structure. In particular, our results imply more large-scale clustering than predicted by popular versions of the Cold Dark Matter cosmogony." @default.
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- W1984652555 date "1990-02-01" @default.
- W1984652555 modified "2023-09-23" @default.
- W1984652555 title "Galaxy correlations on large scales" @default.
- W1984652555 doi "https://doi.org/10.1093/mnras/242.1.43p" @default.
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