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Table 8

Properties of the CIV outflows derived from the outflow component of the CIV emission line.

SDSS Name LCIV Mion ion Ėkin
      
(1045erg s−1) (M) (km s−1) (M yr−1) (1042erg s−1)
      
(1) (2) (3) (4) (5) (6)
      
J0745+4734 1.90 570 4200 7.3 40
J0801+5210 2.6  ± 0.1 770 5050 11.9 100
J0900+4215 1.4  ± 0.1 420 2580 3 7
J0958+2827 0.7  ± 0.2 220 10700 7 260
J1106+6400 2.3  ± 0.1 690 3820 8 40
J1111+1336 2.6  ± 0.2 780 2360 6 10
J1157+2724 0.9  ± 0.1 270 3840 3 15
J1201+0116 0.5  ± 0.1 150 9830 4 130
J1201+1206 1.1  ± 0.1 340 3640 4 20
J1236+6554 2.4  ± 0.1 710 4620 10 68
J13260005 6.9  ± 0.1 2090 1570 10 8
J1421+4633 0.5  ± 0.1 160 10380 5 170
J1422+4417 3.7  ± 0.1 1100 9350 31 870
J1521+5202 1.1  ± 0.1 330 12570 13 630
J1538+0855 1.9  ± 0.1 590 13400 24 1360
J1549+1245 3.8 1070 5230 16 125
J2123–0050 1.2  ± 0.1 350 4720 5 35
J2346–0016 0.5  ± 0.1 150 7580 3 62

Notes. Objects in boldface belong to the [OIII] sample. The following information is listed: (1) SDSS name, (2) CIV luminosity (in units of 1045 erg s−1), (3) ionized gas mass (in units of M), (4) velocityshift of the outflow component (in units of km s−1), (5) ionized gas mass rate (in units of M /yr−1) and (6) kinetic power (units of 1042 erg s−1). (a) We used and in the calculation of the outflow properties of the Weak [OIII] and [OIII] QSOs respectively (see Sect. 4.3.2).

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