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Table C.1

Details of the strong Mg ii systems (Wr ≥ 1 Å) and 21-cm absorption measurements taken from Kanekar et al. (2009).

Quasar zem zabs Wr(Mg iiλ2796) Wr(Mg iiλ2803) Wr(Mg iλ2852) Wr(Fe iiλ2600) ∫τdv Mor. f VLBA cf LS
(Å) (Å) (Å) (Å) (km s-1) (pc)
Systems at 0.5 < z < 1
 B0039 − 407 2.478 0.8485 2.47  ±  0.01V 2.34  ±  0.01 0.56  ±  0.01 1.90  ±  0.01  < 0.49 C1  −   −   − 
 B0109+176 2.157 0.8392 1.75B 1.20  < 0.20 1.09  < 0.039 R2  −   −   − 
 B0240 − 060 1.805 0.5810 1.90  ±  0.02V 1.38  ±  0.02 0.39  ±  0.03 1.70  ±  0.02  < 0.075 C1 1.00 1.00  < 79
1.805 0.7550 1.67  ±  0.01V 1.48  ±  0.01 0.78  ±  0.01 1.25  ±  0.04E1  < 0.061 C1 1.00 1.00  < 88
 B0244 − 128 2.201 0.8282 1.66  ±  0.01V 1.56  ±  0.01 0.49  ±  0.01 1.33  ±  0.01  < 0.13 R3 1.00 0.92 162
 B0409 − 045 1.684 0.8797 1.58  ±  0.22 1.16  ±  0.21  < 0.23 1.21  ±  0.20  < 0.14 C1  −   −   − 
 B0445+097 2.108 0.8392 3.17B 2.19 0.91 1.97  < 0.054 R2 0.22 0.17 80
 B0812+332 2.426 0.8518 2.67  ±  0.28 2.19  ±  0.31 0.55  ±  0.15 1.12  ±  0.27  < 0.11 C 0.07 0.07*  < 30
 B0957+003 0.905 0.6722 1.96  ±  0.16 1.57  ±  0.17 0.32  ±  0.16 1.15  ±  0.24  < 0.06 R  −   −   − 
 B1012+022 1.375 0.7632 1.53  ±  0.05 1.28  ±  0.05 0.33  ±  0.05 0.71  ±  0.05  < 0.06 R  −   −   − 
 B1200+068 2.182 0.862 5.29  ±  0.27 4.88  ±  0.26 3.04  ±  0.27 4.08  ±  0.31  < 0.08 C 1.00 0.66* 170
 B1210+134 1.139 0.7717 1.22  ±  0.09 1.14  ±  0.09 0.38  ±  0.10 0.87  ±  0.10  < 0.052 C? 0.20 0.20  < 74
 B1222+438 1.075 0.7033 1.01  ±  0.25 0.70  ±  0.25  < 0.16 1.22  ±  0.26  < 0.42 R 0.70 0.70  < 72
 B1324 − 047 1.882 0.7850 2.62  ±  0.02V 2.36  ±  0.01 0.78  ±  0.02 1.87  ±  0.02  < 0.48 C? 0.38 0.38  < 75
 B1343+386 1.852 0.8076 1.61  ±  0.12 1.45  ±  0.12  < 0.14 1.20  ±  0.12  < 0.06 R 0.70 0.30* 81
 B1402 − 012 2.518 0.8901 1.14  ±  0.09 1.03  ±  0.09 0.30  ±  0.10 1.08  ±  0.09  < 0.09 C 0.65 0.65  < 78
 B1611+343 1.397 0.6672 1.21  ±  0.06 1.09  ±  0.06  < 0.07 0.58  ±  0.07  < 0.09 C 1.00 1.00  < 70
 B1701+593 1.798 0.7238 1.67  ±  0.22 1.17  ±  0.22 0.80  ±  0.20 1.24  ±  0.24  < 0.10 R  −   −   − 
Systems at 1.1 < z < 1.5
 B1005 − 333 1.837 1.3734 0.93E2 ... ... 0.84  < 0.11 C1 1.00 0.78 280
 B1136+408 2.366 1.3702 1.37  ±  0.21 0.69  ±  0.23  < 0.23 0.60  ±  0.23  < 0.13 C 1.00 1.00? 102
   B1142+052† 1.345 1.3431 2.15  ±  0.11 1.61  ±  0.12 1.29  ±  0.14 1.40  ±  0.17 0.557 R 0.60 0.32 254
 B1204+399 1.518 1.3254 1.41  ±  0.11 1.10  ±  0.11  < 0.11 0.76  ±  0.14  < 0.23 C 1.00 0.72* 564
 B2003 − 025 1.457 1.2116 2.65  ±  0.14A 2.17  ±  0.15  < 0.31 1.27  ±  0.14  < 0.022 R  −   −   − 

Notes. Listed from left to right are the quasar names, their emission redshifts, redshifts of the intervening Mg ii systems, rest frame equivalent widths of the Mg iiλ2796, Mg iiλ2803, Mg iλ2852 and Fe iiλ2600 absorption lines, integrated 21-cm optical depth or in case of non-detection the 3σ upper limit to it for a spectral resolution of 10 km s-1, and quasar morphology at 1.4 GHz. The quasars are classified as compact (C) when deconvolved size in the FIRST is less than 2′′ and resolved (R) when the deconvolved size  > 2′′. When the FIRST is not available, the classification is either based on the radio morphology from the references provided below or on the NVSS/SUMSS when nothing else is available. The last three columns give fVLBA, cf and the largest linear size of the quasars estimated from the milliarcsecond scale resolution maps.

(†)

This system is common with G09.

(V)

Equivalent widths measured using VLT archival spectra.

(B)

Equivalent widths from Barthel et al. (1990).

(Y)

Equivalent widths from York et al. (2007).

(A)

Equivalent widths from Aldcroft et al. (1994).

(E1)

Fe iiλ2600 is not covered in the VLT UVES spectrum, the Wr(Fe iiλ2600) is taken from Ellison et al. (2004).

(E2)

Equivalent widths taken from Ellison et al. (2004).

(1)

Compact on the basis of NVSS/SUMSS.

(2)

Projected linear size  > 2′′ at 5 GHz (Barthel et al. 1988).

(3)

Projected linear size  > 2′′ at 5 GHz (Reid et al. 1999).

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