Table 3: Best-fit parameters and errors. a, b, and c describe the shape of galaxy counts, whereas $\alpha $, $m_{\star }$, and $\Phi _{\star }$ describe the shape of the cluster LF. a, b, c, and $\Phi _{\star }$ are in units of $\rm deg^{-2}$. The last two columns show the half width of the 68% and 95% confidence range, with two degrees of freedom.
  Best-fit 68% 95%
$\alpha $ -0.88 0.09 0.15
$m_{\star }$ 18.66 0.23 0.40
$\Phi_{\star}/10^3$ 3.8    
a 3.19    
b 0.36    
c -0.022    

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