Best-fitting parameters of the warm absorbers (wa1, wa2) and photoionized emission (em) for the RGS spectra. For all these models, ξ is the ionization parameter, σv is the turbulent velocity, NH is the column density and v is the velocity shift with respect to the systemic velocity of NGC 4593; |$N_{\small {em}}$| is the normalization of the photoionized emission table.
| |$\log \xi _{\small {WA}{{1}}}$| (erg s−1 cm) | 2.22 ± 0.01 |
| |$\log \sigma _{v,\small {WA}{{1}}}$| (km s−1) | 1.72 ± 0.07 |
| |$\log N_{\rm{H,}\small {WA}{{1}}}$| (cm−2) | |$21.83 ^{+ 0.07 }_{- 0.02 }$| |
| |$v_{\small {WA}{{1}}}$| (km s−1) | −870 ± 60 |
| |$\log \xi _{\small {WA}{{2}}}$| (erg s−1 cm) | 0.43 ± 0.08 |
| |$\log \sigma _{v,\small {WA}{{2}}}$| (km s−1) | Unconstr. |
| |$\log N_{\rm{H,}\small {WA}{{2}}}$| (cm−2) | 20.90 ± 0.02 |
| |$v_{\small {WA}{{2}}}$| (km s−1) | −300 ± 200 |
| |$\log \xi _{\small {em}}$| (erg s−1 cm) | 0.56 ± 0.03 |
| |$\log \sigma _{v,\small {em}}$| (km s−1) | Unconstr. |
| |$\log N_{\rm{H},\small {em}}$| (cm−2) | >21.4 |
| |$v_{\small {em}}$| (km s−1) | −720 ± 60 |
| |$N_{\small {em}}$| (×10−18) | 6 ± 1 |
| |$\log \xi _{\small {WA}{{1}}}$| (erg s−1 cm) | 2.22 ± 0.01 |
| |$\log \sigma _{v,\small {WA}{{1}}}$| (km s−1) | 1.72 ± 0.07 |
| |$\log N_{\rm{H,}\small {WA}{{1}}}$| (cm−2) | |$21.83 ^{+ 0.07 }_{- 0.02 }$| |
| |$v_{\small {WA}{{1}}}$| (km s−1) | −870 ± 60 |
| |$\log \xi _{\small {WA}{{2}}}$| (erg s−1 cm) | 0.43 ± 0.08 |
| |$\log \sigma _{v,\small {WA}{{2}}}$| (km s−1) | Unconstr. |
| |$\log N_{\rm{H,}\small {WA}{{2}}}$| (cm−2) | 20.90 ± 0.02 |
| |$v_{\small {WA}{{2}}}$| (km s−1) | −300 ± 200 |
| |$\log \xi _{\small {em}}$| (erg s−1 cm) | 0.56 ± 0.03 |
| |$\log \sigma _{v,\small {em}}$| (km s−1) | Unconstr. |
| |$\log N_{\rm{H},\small {em}}$| (cm−2) | >21.4 |
| |$v_{\small {em}}$| (km s−1) | −720 ± 60 |
| |$N_{\small {em}}$| (×10−18) | 6 ± 1 |
Best-fitting parameters of the warm absorbers (wa1, wa2) and photoionized emission (em) for the RGS spectra. For all these models, ξ is the ionization parameter, σv is the turbulent velocity, NH is the column density and v is the velocity shift with respect to the systemic velocity of NGC 4593; |$N_{\small {em}}$| is the normalization of the photoionized emission table.
| |$\log \xi _{\small {WA}{{1}}}$| (erg s−1 cm) | 2.22 ± 0.01 |
| |$\log \sigma _{v,\small {WA}{{1}}}$| (km s−1) | 1.72 ± 0.07 |
| |$\log N_{\rm{H,}\small {WA}{{1}}}$| (cm−2) | |$21.83 ^{+ 0.07 }_{- 0.02 }$| |
| |$v_{\small {WA}{{1}}}$| (km s−1) | −870 ± 60 |
| |$\log \xi _{\small {WA}{{2}}}$| (erg s−1 cm) | 0.43 ± 0.08 |
| |$\log \sigma _{v,\small {WA}{{2}}}$| (km s−1) | Unconstr. |
| |$\log N_{\rm{H,}\small {WA}{{2}}}$| (cm−2) | 20.90 ± 0.02 |
| |$v_{\small {WA}{{2}}}$| (km s−1) | −300 ± 200 |
| |$\log \xi _{\small {em}}$| (erg s−1 cm) | 0.56 ± 0.03 |
| |$\log \sigma _{v,\small {em}}$| (km s−1) | Unconstr. |
| |$\log N_{\rm{H},\small {em}}$| (cm−2) | >21.4 |
| |$v_{\small {em}}$| (km s−1) | −720 ± 60 |
| |$N_{\small {em}}$| (×10−18) | 6 ± 1 |
| |$\log \xi _{\small {WA}{{1}}}$| (erg s−1 cm) | 2.22 ± 0.01 |
| |$\log \sigma _{v,\small {WA}{{1}}}$| (km s−1) | 1.72 ± 0.07 |
| |$\log N_{\rm{H,}\small {WA}{{1}}}$| (cm−2) | |$21.83 ^{+ 0.07 }_{- 0.02 }$| |
| |$v_{\small {WA}{{1}}}$| (km s−1) | −870 ± 60 |
| |$\log \xi _{\small {WA}{{2}}}$| (erg s−1 cm) | 0.43 ± 0.08 |
| |$\log \sigma _{v,\small {WA}{{2}}}$| (km s−1) | Unconstr. |
| |$\log N_{\rm{H,}\small {WA}{{2}}}$| (cm−2) | 20.90 ± 0.02 |
| |$v_{\small {WA}{{2}}}$| (km s−1) | −300 ± 200 |
| |$\log \xi _{\small {em}}$| (erg s−1 cm) | 0.56 ± 0.03 |
| |$\log \sigma _{v,\small {em}}$| (km s−1) | Unconstr. |
| |$\log N_{\rm{H},\small {em}}$| (cm−2) | >21.4 |
| |$v_{\small {em}}$| (km s−1) | −720 ± 60 |
| |$N_{\small {em}}$| (×10−18) | 6 ± 1 |
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