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Table 1

CO and H2 content of strong C I absorbers.

Quasar zabs logN (cm−2) Ref.
C I CO H2
J0216−0021 1.737 14.25 ± 0.02 <12.97 1
J0300−0721 1.536 >14.77 ≤13.79 1
J0811+0838 1.906 13.68 ± 0.13 <13.24 1
J0815+2640 1.681 >14.73 <13.68 1
J0820+1559 1.547 >14.71 <14.01 1
J0852+1935 1.788 15.01 ± 0.12 <13.33 1
J0854+0317 1.567 14.23 ± 0.01 <13.11 1
J0857+1855 1.730 14.57 ± 0.13 13.54 ± 0.05 2
J0917+0154 2.107 14.32 ± 0.06 <14.07 1
J0927+1543 1.731 >14.61 <13.32 1
J1047+2057 1.775 >14.90 14.40 ± 0.07 2
J1117+1437 2.001 14.40 ± 0.03 <13.13 ~18 1
J1122+1437 1.554 13.83 ± 0.03 <12.99 1
J1129−0237 1.623 >14.96 <13.31 1
J1133−0057 1.706 15.12 ± 0.06 ≤14.07 1
J1237+0647 2.691 15.01 ± 0.02 14.17 ± 0.09 3
J1248+2848 1.513 14.25 ± 0.10 <13.25 1
J1302+2111 1.656 14.30 ± 0.02 <13.48 1
J1306+2815 2.012 14.47 ± 0.04 <13.26 1
J1311+2225 3.092 14.30 ± 0.02 <13.43 1
J1314+0543 1.583 14.40 ± 0.02 ≤13.77 1
J1341+1852 1.544 13.51 ± 0.03 <13.00 1
J1346+0644 1.512 14.51 ± 0.02 <13.60 1
J1439+1117 2.418 14.81 ± 0.02 13.89 ± 0.02 4
J1459+0129 1.623 14.32 ± 0.09 <13.57 1
J1522+0830 1.627 >14.47 <13.50 1
J1603+1701 1.890 13.80 ± 0.10 <12.88 1
J1604+2203 1.641 >15.14 14.59 ± 0.11 5
J1615+2648 2.118 14.49 ± 0.06 <13.16 1
J1623+1355 1.751 14.41 ± 0.07 <13.30 1
J1646+2329 1.998 14.32 ± 0.06 <13.40 1
J1705+3543 2.038 >15.01 14.14 ± 0.03 2
J2123−0050 2.060 14.11 ± 0.02 <13.07 1,6
J2229+1414 1.586 13.96 ± 0.05 <13.55 1
J2257−1001 1.836 14.65 ± 0.01 <13.09 19.5 ± 0.1 1
J2331−0908 2.143 >14.70 13.65 ± 0.03 1
J2336−1058 1.829 14.07 ± 0.02 <12.93 1
J2340−0053 2.054 14.09 ± 0.04 <12.58 1,7
J2350−0052 2.426 14.36 ± 0.01 <12.94 1,8

References. The references listed in the last column are for molecular measurements. When two references are listed, they correspond to CO then H2, in this order. (1) This work; (2) Noterdaeme et al. (2011); (3) Noterdaeme et al. (2010); (4) Srianand et al. (2008); (5) Noterdaeme et al. (2009); (6) Klimenko et al. (2016); (7) Jorgenson et al. (2010); (8) Noterdaeme et al. (2007). Unless already available from the literature, C I column densities were obtained through the apparent optical depth method.

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