2005MNRAS.360.1244A

We present measurements of the clustering properties of bright (L > L_*) z∼ 4 Lyman break galaxies (LBGs) selected from the Oxford-Dartmouth Thirty Degree Survey (ODT). We describe techniques used to select and evaluate our candidates and calculate the angular correlation function, which we find best fitted by a power law, ω(θ) =A_wθ^–β with A_w= 15.4 (with θ in arcsec), using a constrained slope of β= 0.8. Using a redshift distribution consistent with photometric models, we deproject this correlation function and find a comoving r₀= 11.4^+1.7_–1.9h^–1₁₀₀Mpc in a Ω_m= 0.3 flat Λ cosmology for i_AB≤ 24.5. This corresponds to a linear bias value of b= 8.1^+2.0_–2.6(assuming σ₈= 0.9). These data show a significantly larger r₀and b than previous studies at z∼ 4. We interpret this as evidence that the brightest LBGs have a larger bias than fainter ones, indicating a strong luminosity dependence for the measured bias of an LBG sample. Comparing this against recent results in the literature at fainter (subL_*) limiting magnitudes, and with simple models describing the relationship between LBGs and dark matter haloes, we discuss the implications on the implied environments and nature of LBGs. It seems that the brightest LBGs (in contrast with the majority subL_*population) have clustering properties, and host dark matter halo masses, which are consistent with them being progenitors of the most massive galaxies today.