Extended Data Table 1 Sample selection and the corresponding results

From: Unexpected clustering pattern in dwarf galaxies challenges formation models

  1. The columns show the values of the corresponding quantities, with uncertainties corresponding to the 16th and 84th percentiles. The uncertainties are rounded to two decimal places, and a value of 0.0 represents the uncertainty of less than 0.004. Column a: Median stellar mass of the sample; Column b: Halo mass estimated from SHMR; Column c: Halo mass measured from HI-kinematics; Column d: Relative bias obtained using the z-matching method; Column e: Relative bias obtained using the z-weighting method; Column f: Theoretical halo bias of the sample.
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