Table 1
Properties of the three quasars from literature.
| Ionised outflow properties | ||||||||||
| QSO | z | RA | Dec | Log10( |
M BH | SFR | v | R | M [ OIII ] | Ṁ [ OIII ] |
| [1010M⊙] | [M⊙ yr-1] | [km s-1] | [kpc] | [107M⊙] | [M⊙ yr-1] | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
|
|
||||||||||
| LBQS0109 | 2.35 | 01:12:16.99 | +02:29:47.7 | 47.5 | 1.0 | 50 | 1850 | 0.4 | 1.2 | 60 |
| 2QZJ0028 | 2.40 | 00:28:30.42 | –28:17:05.4 | 47.3 | 1.2 | 100 | 2300 | 0.7 | 3.8 | 140 |
| HB8903 | 2.44 | 03:31:06.41 | –38:24:04.6 | 47.5 | 1.3 | 90 | 1450 | 1.9 | 0.7 | 6 |
Notes. (1) ID of the object. (2) Redshifts estimated from the narrow [Oiii]λ5007 emission (Carniani et al. 2015b). (3, 4) Coordinates (J2000.0). (5) AGN bolometric luminosities derived by using the relation LAGN~ 6 λL(λ5100Å) from Marconi et al. (2004). (6) Black hole masses from Shemmer et al. (2004) and Williams et al. (2017). (7) SFR estimated from Hα emission (Carniani et al. 2016). (8, 9) [Oiii]λ5007 Outflow velocity and inferred by using the spectro-astrometric method described in Carniani et al. (2015b). (10) Outflow masses inferred from [Oiii]λ5007 by assuming Te ~ 104 K and ne ~ 500 cm-3. (11) Outflow mass-loss rates calculated as Ṁo = Mo/τdyn = Movo/Ro.
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