2013

Galaxy Assembly Bias: A Significant Source of Systematic Error in the Galaxy-Halo Relationship

Zentner, Andrew R., Hearin, Andrew P., Bosch, Frank C. van den

Understand

It is common practice for methods that use galaxy clustering to constrain the galaxy-halo relationship, such as the halo occupation distribution (HOD) and/or conditional luminosity function (CLF), to assume that halo mass alone suffices to determine a halo's resident galaxy population.

  • Yet, the clustering strength of cold dark matter halos depends upon halo properties in addition to mass, such as formation time, an effect referred to as assembly bias.
  • If galaxy characteristics are correlated with any of these auxiliary halo properties, the basic assumption of HOD/CLF methods is violated.
  • We estimate the potential for assembly bias to induce systematic errors in inferred halo occupation statistics.

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