Table 3: Rest-frame properties inferred for the two sources dominated by stellar light.
Source LK $M_{\rm star}$ $M_{\rm BH}^{\rm a}$ $L/L_{\rm Edd}^{\rm b}$
  $(L_{\odot})$ $(M_{\odot})$ $(M_{\odot})$  
BPM16274#069 $\rm 8.3\times 10^{11}$ $\rm 4\times 10^{11}$ $\rm 2\times 10^9$ 0.04
Abell2690#075 $\rm 1.7\times10^{12}$ $8 \times 10^{11}$ $\rm 3\times 10^9$ 0.10
Notes: a Inferred black hole mass assuming the $L_{\rm K}-M_{\rm BH}$ relation obtained by Marconi & Hunt (2003) for local galaxies. b Eddington ratio assuming a bolometric correction $L_{\rm bol}/L_{\rm X}=30$.

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