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We investigate the galaxy clustering, bias and HOD dependence on the [OII] emission-line luminosity in the local Universe

Clustering measurements + SHAM models:

Screenshot 2023-09-20 at 00.57.27.png
quadmodelELG.jpg
wpELGmodel.jpg

SHAM-inferred HOD shape:

HOD_ELGs.jpg

ELG bias VS [OII] luminosity:

biaswpELG.jpg
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