Fig. 2
MBH − Mstar relation for AGNs at z ~ 1–2. The red diamonds with errorbars show the location of the three X-ray selected obscured AGNs presented in this paper. Green triangles are type 1, X-ray selected unobscured AGNs in COSMOS from Merloni et al. (2010). Blue squares are obscured AGNs in SMGs from Alexander et al. (2008) with broad Hα and stellar masses from Hainline et al. (2010). The black line is the local relation obtained by Sani et al. (2010).
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