Based on observations collected at the European Southern Observatory (ESO), La Silla, Chile.

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All appendices are only available in electronic form at http://www.aanda.org

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... indistinguishable

The late spiral versus early-type cross-correlation function might be smoother than the dwarf versus late spiral cross-correlation because there are 72% more early-type galaxies than dwarf galaxies in the considered samples (see Table 1).

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