| . | |$\log L_{\rm bol} ^{a }$| . | |$\rm logM_{BH}$| . | |$\rm \lambda _{Edd}$| . | |$\log L_{\rm X}^{b}$| . | |$\rm logN_{H}$| . | Γ . |
|---|---|---|---|---|---|---|
| . | |$\rm (erg\, s^{-1})$| . | (M⊙) . | . | |$\rm (erg\, s^{-1})$| . | |$\rm (cm^{-2})$| . | . |
| a2 | 45.4 ± 0.2 | |$7.55 _{-0.38} ^{+0.35}$| | |$0.51 _{-0.35} ^{+0.68}$| | 44.0 | ≳ 23.8 | 1.9 |
| b1 | 45.6 ± 0.2 | |$7.86 _{-0.37}^{+0.34}$| | |$0.46_{-0.30} ^{+0.57}$| | 44.1 | 22.7 | 1.4 ± 0.2 |
| . | |$\log L_{\rm bol} ^{a }$| . | |$\rm logM_{BH}$| . | |$\rm \lambda _{Edd}$| . | |$\log L_{\rm X}^{b}$| . | |$\rm logN_{H}$| . | Γ . |
|---|---|---|---|---|---|---|
| . | |$\rm (erg\, s^{-1})$| . | (M⊙) . | . | |$\rm (erg\, s^{-1})$| . | |$\rm (cm^{-2})$| . | . |
| a2 | 45.4 ± 0.2 | |$7.55 _{-0.38} ^{+0.35}$| | |$0.51 _{-0.35} ^{+0.68}$| | 44.0 | ≳ 23.8 | 1.9 |
| b1 | 45.6 ± 0.2 | |$7.86 _{-0.37}^{+0.34}$| | |$0.46_{-0.30} ^{+0.57}$| | 44.1 | 22.7 | 1.4 ± 0.2 |
a derived from |$L_{5100\, \mathrm{\mathring{\rm A}}|}$| following Runnoe et al. (2012)
b the values of |$\log L_{\rm [2-10]\, keV}$| reported are intrinsic (unabsorbed). This value has been computed from the X-ray spectrum for b1, while for a2 has been derived from the bolometric luminosity.
| . | |$\log L_{\rm bol} ^{a }$| . | |$\rm logM_{BH}$| . | |$\rm \lambda _{Edd}$| . | |$\log L_{\rm X}^{b}$| . | |$\rm logN_{H}$| . | Γ . |
|---|---|---|---|---|---|---|
| . | |$\rm (erg\, s^{-1})$| . | (M⊙) . | . | |$\rm (erg\, s^{-1})$| . | |$\rm (cm^{-2})$| . | . |
| a2 | 45.4 ± 0.2 | |$7.55 _{-0.38} ^{+0.35}$| | |$0.51 _{-0.35} ^{+0.68}$| | 44.0 | ≳ 23.8 | 1.9 |
| b1 | 45.6 ± 0.2 | |$7.86 _{-0.37}^{+0.34}$| | |$0.46_{-0.30} ^{+0.57}$| | 44.1 | 22.7 | 1.4 ± 0.2 |
| . | |$\log L_{\rm bol} ^{a }$| . | |$\rm logM_{BH}$| . | |$\rm \lambda _{Edd}$| . | |$\log L_{\rm X}^{b}$| . | |$\rm logN_{H}$| . | Γ . |
|---|---|---|---|---|---|---|
| . | |$\rm (erg\, s^{-1})$| . | (M⊙) . | . | |$\rm (erg\, s^{-1})$| . | |$\rm (cm^{-2})$| . | . |
| a2 | 45.4 ± 0.2 | |$7.55 _{-0.38} ^{+0.35}$| | |$0.51 _{-0.35} ^{+0.68}$| | 44.0 | ≳ 23.8 | 1.9 |
| b1 | 45.6 ± 0.2 | |$7.86 _{-0.37}^{+0.34}$| | |$0.46_{-0.30} ^{+0.57}$| | 44.1 | 22.7 | 1.4 ± 0.2 |
a derived from |$L_{5100\, \mathrm{\mathring{\rm A}}|}$| following Runnoe et al. (2012)
b the values of |$\log L_{\rm [2-10]\, keV}$| reported are intrinsic (unabsorbed). This value has been computed from the X-ray spectrum for b1, while for a2 has been derived from the bolometric luminosity.
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