Key points are not available for this paper at this time.
We revisit the longstanding question of whether first brightest cluster galaxies (BCGs) are statistically drawn from the same distribution as other cluster galaxies or are 'special', using the new non-parametric, empirically based, model presented in Vale & Ostriker for associating galaxy luminosity with halo/subhalo masses.
Vale et al. (Tue,) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: