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Table 3

Properties of the compiled sample of dusty QSO-DLAs.

Source zQSO zDLA AV log N(H I) [X/H] X [Fe/X] Survey References
(mag) (cm−2)
J 0000+0048 3.028 2.525 0.23 20.80 ± 0.10   0.46 ± 0.45 Zn − 1.89 ± 0.50 BOSSa,b (1)
J 0016–0012 2.092 1.970 0.11 20.75 ± 0.15 − 0.86 ± 0.13 * − 0.99 ± 0.10 BOSSa (2)
eHAQ 0111+0641 3.214 2.027 0.22 21.50 ± 0.30 − 0.60 ± 0.30 Zn − 0.60 ± 0.10 eHAQc (3,4)
J 0316+0040 2.911 2.180 0.12 21.10 ± 0.20 − 1.20 ± 0.22 * − 0.63 ± 0.20 SEGUE2d (2)
J 0812+3208 2.711 2.626 0.11 21.35 ± 0.15 − 0.88 ± 0.11 * − 0.15 ± 0.05 BOSSa,e (2)
J 0816+1446 3.847 3.287 0.15 22.00 ± 0.10 − 1.10 ± 0.10 Zn − 0.48 ± 0.02 BOSSa (5)
J 0840+4942 2.090 1.851 0.13 20.75 ± 0.15 − 0.43 ± 0.17 * − 0.71 ± 0.15 SDSS⋆,f (2)
Q 0918+1636 3.070 2.583 0.22 20.96 ± 0.05 − 0.12 ± 0.05 Zn − 0.91 ± 0.08 BOSS⋆,a,b,g (6)
J 0927+5823 1.910 1.635 0.38 20.40 ± 0.25 − 0.22 ± 0.25 * BOSSe (2)
J 1135–0010 2.888 2.207 0.11 22.10 ± 0.05 − 1.10 ± 0.20 Zn − 0.72 ± 0.10 BOSS⋆,a,g,i,j (7)
J 1157+6155 2.513 2.460 0.59 21.80 ± 0.20 − 0.60 ± 0.38 Zn − 1.02 ± 0.47 SDSS⋆,h (8,9)
J 1211+0833 2.483 2.117 0.53 21.00 ± 0.20 − 0.07 ± 0.21 Zn − 1.74 ± 0.25 BOSS⋆,g,j (10)
J 1310+5424 1.929 1.801 0.27 21.45 ± 0.15 − 0.51 ± 0.15 * SDSS⋆,f,h (2)
KV-RQ 1500–0013 2.520 2.428 0.16 21.20 ± 0.10 − 0.90 ± 0.20 * KV-RQc This work
J 1709+3258 1.889 1.830 0.17 20.95 ± 0.15 − 0.28 ± 0.15 * − 0.53 ± 0.15 BOSSk (2)
Q 2222+0946 2.927 2.354 0.15 20.55 ± 0.15 − 0.46 ± 0.07 Zn − 0.77 ± 0.05 SDSS⋆,f,l (2,11)
HAQ 2225+0527 2.320 2.130 0.28 20.69 ± 0.05 − 0.09 ± 0.05 Zn − 1.22 ± 0.06 HAQc (12,13)
J 2340–0053 2.084 2.055 0.19 20.35 ± 0.15 − 0.59 ± 0.15 * − 0.53 ± 0.12 BOSSe (2,8)

Notes. Selection flags given in the SDSS database: (a)Known QSO at z > 2.15; (b)Additional object observed to reach 40 QSOs deg−1 for BOSS outside the standard selection criteria; (c)Red optical to near/mid-infrared selection, classified as star in SDSS/BOSS; (d)Classified as a star in the SEGUE-2 survey; (e)FIRST radio selected; (f)Bright ugri-selected quasar; (g)Identified by the neural network and the kernel density estimation (KDE) plus χ2 algorithms of BOSS; (h)High-redshift griz-selected quasar; (i)Identified by the BOSS likelihood method; (j)Selected to be in the uniform BOSS core sample; (k)Filler target; (l)Classified as a blue horizontal branch star as part of the SEGUE target selection. (⋆)Quasars selected from the photometric selection criteria and identification algorithms defined specifically for the SDSS/BOSS surveys. (*)Metallicities from Kaplan et al. (2010) are either based on Si II, Zn II or S II, but the exact ion is not listed in their table 2, and for KV-RQ 1500–0013 the metallicity is derived from an empirical relation based on the equivalent width of Si II λ 1526. (1) Noterdaeme et al. (2017); (2) Kaplan et al. (2010); (3) Krogager et al. (2016a); (4) Fynbo et al. (2017); (5) Guimarães et al. (2012); (6) Fynbo et al. (2011); (7) Noterdaeme et al. (2012a); (8) Ledoux et al. (2015); (9) Wang et al. (2012); (10) Ma et al. (2015); (11) Fynbo et al. (2010); (12) Krogager et al. (2015); (13) Krogager et al. (2016b).

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