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Bolometric luminosities: Lx+L(IR)
Eddington ratios : Lbol/MBH
MBH: from EW of broad lines (type1)
MBH: estimation from host galaxy bulge
sample size: ~1000
LIR from Herschel-PACS bands
bolometric correction Lbol/L[0.5-2.0kev] is larger for Lbol：越高Lx光度的AGN，LIR/Lx越大