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Classification of Extremely Red Objects in the Cosmos Field

  • Authors: Xu Kong, Guanwen Fang, Nobuo Arimoto, and Min Wang

KONG et al. 2009 The Astrophysical Journal 702 1458.

  • Provider: AAS Journals

Caption: Figure 6.

Gini coefficient ( G) vs. central concentration ( C) for EROs. The solid line corresponds to unity slope, the big squares show the median value of G at different C bins, from 0.2 to 0.55. The dashed lines are ±10% offset relative to the solid line.

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