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Table 2.

Parameters of the sources observed with MeerKAT.

Source Stot log Ltot Score ΔSpeak τpeak S dv W50 W20 W0 NH I Morph LUV 1216 Å
(Jy) (W Hz−1) (Jy) (mJy) (10−3) (mJy km s−1) (km s−1) (km s−1) (km s−1) (1020 cm−2) (1023 W Hz−1)
0159–11 3.615 28.05 3.280 < 0.59 < 0.07 E 120
0252–71 8.879 28.24 8.879 < 0.59 < 0.07 U 0.02
0403–13 4.964 28.00 4.964 < 0.51 < 0.09 U 1.9
0405–12 4.132 27.93 0.839a 4.5 ± 1.0b 4.76 372 ± 29 90 ± 20 125 ± 30 160 ± 20 0.81 E 22
0637–75 6.938 28.30 4.980 < 0.64 < 0.12 E 9.5
0842–75 E 17
0859–25 7.539 27.45 E 0.07
1136–13 6.332 28.00 2.280 < 1.20 < 0.22 E 3.8
1151–34 7.498 27.27 7.498 28.0 ± 2.0 4.0 5386 ± 105 157 ± 20 350 ± 25 450 ± 30 1.31 U 0.18
1306–09 5.429 27.79 5.429 4.5 ± 1.0 0.9 1072 ± 69 260 ± 30 405 ± 30 455 ± 30 0.36 U 0.08
1355–41 5.905 27.38 0.115 < 17.1 < 3.11 E 4.2
1510–08 3.332 27.29 1.470 < 1.41 < 0.26 E 0.60
1602+01 6.418 27.86 3.220 < 0.90 < 0.16 E 0.81
1954–388 1.195 27.50 0.947 < 1.74 < 0.32 E 1.20
2203–18 7.288 28.26 7.288 < 0.49 < 0.09 U 0.04
2243–123 1.692 27.65 1.580 < 1.12 < 0.20 E 2.10
2345–16 2.602 27.73 2.602 < 0.89 < 0.16 U 0.71

Notes. The continuum fluxes are obtained at the frequency of the H I observations; therefore, at 1.4 GHz in the rest frame at the redshift of the source and it is the same for the total luminosities. The column densities are assuming Tspin = 100 K and a covering factor cf = 1. The upper limits to the column density are estimated using the 3-σ noise and a FWHM of the line of 100 km s−1. (a)Flux of the peak of the southern lobe. (b)Absorption against the southern lobe.

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