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- W458030 abstract "As part of a larger study of the clustering properties of galaxies at intermediate redshifts, we present a study of methods and algorithms used to estimate the angular correlation function, ω(θ), of faint galaxies. A technique has been developed which permits the reliable measurement of ω(θ) at amplitude levels as low as ∼0.002 for fields of area ∼2 deg 2 - i.e. to separations of order 1 degree for galaxies with a blue magnitude ≃+24. An iterative method has been used to compute the best mean density that ensures consistency between the integral constraint and ω(θ). Artificial galaxy catalogues with built in correlation functions have been analyzed to test for the presence of spurious correlations associated with, for example, field geometry" @default.
- W458030 created "2016-06-24" @default.
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- W458030 date "1994-02-01" @default.
- W458030 modified "2023-09-24" @default.
- W458030 title "Correlation analysis of faint galaxies" @default.
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