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The clustering of H β + [O III] and [O II] emitters since z ∼ 5:dependencies with line luminosity and stellar mass

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Figure

Figure 1. The full COSMOS and UDS on-sky coverages with the NBJ filter. Shown inHand clearly outline the masked regions which are associated with bright stars and artifacts
Figure 2. The angular correlation function based on the medianLimber approximation fits
Figure 3. The angular correlation function for ther[OFigure z = 1.47ii] sample. Shown are the observed w(θ) measurements as in 2 with the corresponding Limber approximation and ex-act Limber equation fits
Table 1. The clustering properties for our Husing the exact Limber equation as defined in Equationfixed toto the clustering amplitude,β+[Oiii] and [Oii] samples
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