Table 1.
X-ray properties, stellar mass and outflow properties of our candidates with outflows.
| EROID | log NH | log LX | log Lbol | log M* | Rout | Mout | Ṁ | Ė | ṖOF |
|---|---|---|---|---|---|---|---|---|---|
| (cm−2) | (erg s−1) | (erg s−1) | (M⊙) | (kpc) | (M⊙ 106) | (M⊙ yr−1) | (erg s−1 1041) | (dyne 1034) | |
| 25592 | 20.3 | 42.7 | 43.9 | 11.2 | 5.4 | 10.7 ± 0.1 | 17.1 ± 0.3 | 241.9 ± 8.4E–6 | 22.9 |
| 6743 | 23.0 | 44.2 | 45.5 | 10.8 | 6.5 | 0.8 ± 0.03 | 0.6 ± 0.06 | 2.6 ± 9.4E–5 | 0.4 |
| 608 | 22.3 | 44.8 | 46.2 | −99.0 | 10.0 | 4.4 ± 0.2 | 2.6 ± 0.1 | 17.2 ± 8.4E–5 | 2.4 |
| 19520 | 22.1 | 44.0 | 45.3 | 9.8 | 4.5 | 13.0 ± 0.9 | 22.6 ± 2.2 | 260.6 ± 0.005 | 27.3 |
| 18777 | 21.5 | 43.7 | 44.9 | 10.9 | 9.0 | 1.8 ± 0.1 | 2.7 ± 0.3 | 94.7 ± 0.005 | 5.7 |
| 21835* | 21.8 | 44.3 | 45.6 | 10.9 | 9.3 | 6.3 ± 0.5 | 2.1 ± 0.3 | 4.2 ± 6.2E–4 | 1.1 |
| 12686 | 22.4 | 44.3 | 45.6 | 10.9 | 6.0 | 4.1 ± 0.3 | 3.1 ± 0.6 | 12.0 ± 0.006 | 2.2 |
| 31136 | 21.7 | 43.1 | 44.3 | −99.0 | 10.0 | 4.5 ± 0.4 | 2.9 ± 0.3 | 24.0 ± 8.7E–4 | 3.0 |
| 5896* | 22.3 | 44.4 | 45.7 | −99.0 | 10.0 | 9.1 ± 0.9 | 3.4 ± 0.5 | 8.9 ± 0.001 | 2.0 |
| 16271 | 21.7 | 43.5 | 44.7 | 10.3 | 2.0 | 0.6 ± 0.09 | 1.5 ± 0.3 | 7.3 ± 0.007 | 1.2 |
| 14896 | 21.5 | 43.9 | 45.2 | 11.2 | 3.5 | 1.7 ± 0.2 | 2.5 ± 0.5 | 13.9 ± 0.008 | 2.1 |
| 10152 | 20.7 | 43.8 | 45.1 | −99.0 | 10.0 | 2.2 ± 0.3 | 1.9 ± 0.9 | 27.4 ± 0.4 | 2.6 |
| 11596 | 21.6 | 44.2 | 45.5 | 10.9 | 3.9 | 7.3 ± 1.3 | 20.2 ± 4.0 | 452.4 ± 0.04 | 34.0 |
| 14390 | 21.7 | 43.5 | 44.7 | 10.2 | 3.0 | 5.7 ± 1.1 | 6.4 ± 1.3 | 13.7 ± 5.4E–4 | 3.3 |
| 16050 | 21.6 | 43.5 | 44.8 | 11.1 | 7.7 | 2.8 ± 0.6 | 1.4 ± 0.6 | 3.9 ± 0.04 | 0.8 |
| 19964 | 21.7 | 43.5 | 44.8 | 10.5 | 5.7 | 0.4 ± 0.1 | 0.1 ± 0.06 | 0.1 ± 4.7E–4 | 0.1 |
| 14541 | 21.5 | 43.8 | 45.1 | 10.0 | 4.6 | 2.1 ± 0.6 | 6.8 ± 2.9 | 274.6 ± 2.5 | 15.4 |
| 19174 | 22.9 | 44.4 | 45.7 | 11.0 | 5.7 | 12.3 ± 3.9 | 11.9 ± 8.7 | 70.1 ± 6.3 | 10.3 |
| 28337 | 21.9 | 43.9 | 45.2 | −99.0 | 2.9 | 1.0 ± 0.3 | 0.7 ± 0.5 | 0.7 ± 0.04 | 0.3 |
| 16799 | 21.6 | 43.3 | 44.5 | 10.8 | 7.8 | 0.6 ± 0.2 | 0.1 ± 0.2 | 0.1 ± 0.1 | 0.04 |
| 19841 | 21.5 | 43.6 | 44.9 | −99.0 | 10.0 | 1.5 ± 0.5 | 0.4 ± 0.1 | 0.9 ± 7.1E–4 | 0.2 |
| 17754 | 21.7 | 44.1 | 45.3 | 10.9 | 6.3 | 0.5 ± 0.1 | 0.2 ± 0.1 | 0.6 ± 0.004 | 0.1 |
| 15417 | 22.1 | 44.1 | 45.4 | 10.3 | 7.8 | 9.9 ± 3.5 | 6.2 ± 2.3 | 28.1 ± 0.02 | 4.7 |
Notes. The columns (left-right) are eROSITA ID (EROID) of our candidates with outflows, column density (log NH), X-ray luminosity (LX; 2−10 keV), AGN bolometric luminosity (AGN Lbol) and stellar mass (M*). Column density and X-ray luminosity are obtained from Liu et al. (2022), AGN bolometric luminosity calculated from X-ray luminosity and the bolometric corrections using Eq. (3) in Duras et al. (2020) relation. Followed by outflow properties; radius (Rout), outflow mass (Mout), mass outflow rate (Ṁ), outflow kinetic power (Ė) and momentum flux of the outflow (ṖOF) as estimated in this study. −99.0 is used to indicate missing values. Sources marked with * have single Gaussian components.
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