Table 9: Luminous and dark mass measurements of the lens galaxy, without the cluster contribution. The ranges represent the intervals at 68% confidence level.
  $M_{{\rm len}}$ $M_{{\rm dyn}}$ $M_{{\rm phot}}$ $f_{{\rm DM}}$
  $(10^{11}~M_{\odot})$ $(10^{11}~M_{\odot})$ $(10^{11}~M_{\odot})$  
$R\leq8.10$ kpc 3.9-5.2 2.8-4.0 0.6-0.9 0.44-0.99
$R\leq9.54$ kpc 4.6-6.2 3.3-4.7 0.7-1.1 0.50-0.99

Source LaTeX | All tables | In the text