Table 1.
Source identification and basic properties of the GTC-xA quasars.
SDSS identification | z | Δz | Line | mv | MB | g − r | Comments |
---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
SDSSJ000807.27-103942.7 | 2.4660 | 0.0010 | III | 19.15 | –26.2 | 0.08 | |
SDSSJ004241.95+002213.9 | 2.0560 | 0.0053 | III | 19.05 | –25.6 | 0.24 | |
SDSSJ021606.41+011509.5 | 2.2236 | 0.0008 | I,II | 19.36 | –25.2 | 0.49 | BAL |
SDSSJ024154.42-004757.5 | 2.3919 | 0.0015 | III | 19.24 | –26.0 | 0.24 | |
SDSSJ084036.16+235524.7 | 2.1879 | 0.0012 | III | 19.46 | –25.3 | 0.40 | |
SDSSJ101822.96+203558.6 | 2.2502 | 0.0035 | III | 19.27 | –25.5 | 0.33 | |
SDSSJ103527.40+445435.6 | 2.2639 | 0.0060 | III | 19.34 | –25.6 | 0.20 | |
SDSSJ105806.16+600826.9 | 2.9406 | 0.0001 | I,II | 19.29 | –26.7 | 0.16 | |
SDSSJ110022.53+484012.6 | 2.0884 | 0.0028 | III | 18.90 | –25.9 | 0.13 | |
SDSSJ125659.79-033813.8 | 2.9801 | 0.0004 | II | 19.27 | –26.7 | 0.26 | BAL |
SDSSJ131132.92+052751.2 | 2.1234 | 0.0009 | III | 19.06 | –25.4 | 0.72 | BAL |
SDSSJ143525.31+400112.2 | 2.2615 | 0.0006 | III | 18.30 | –26.6 | 0.17 | |
SDSSJ144412.37+582636.9 | 2.3455 | 0.0018 | III | 19.21 | –25.8 | 0.37 | Mini–BAL |
SDSSJ151258.36+352533.2 | 2.2382 | 0.0012 | III | 19.21 | –25.8 | 0.04 | RL, logPν ≈ 33.8, log![]() |
SDSSJ214009.01-064403.9 | 2.0808 | 0.0038 | III | 19.26 | –25.3 | 0.56 | BAL |
SDSSJ220119.62-083911.6 | 2.1840 | 0.0015 | III | 18.68 | –26.1 | 0.35 | BAL |
SDSSJ222753.07-092951.7 | 2.1639 | 0.0010 | III | 19.11 | –25.6 | 0.10 | |
SDSSJ233132.83+010620.9 | 2.6271 | 0.0038 | III | 19.19 | –26.1 | 0.33 | RL, logPν ≈ 34.1, log![]() |
SDSSJ234657.25+145736.0 | 2.1682 | 0.0007 | III | 19.11 | –25.7 | 0.29 | RI, logPν ≈ 32.7, log![]() |
Notes. Columns are as follows: (1) SDSS coordinate name. (2) Redshift. (3) Redshift uncertainty. (4) Lines used for redshift determination: I: C II1335, II: OI+SiII λ1305, III: Al IIIλ1860 +Si III]
1892. (5) Apparent Johnson V magnitude as reported by Véron-Cetty & Véron (2010). (6) Absolute B magnitude according to Véron-Cetty & Véron (2010). (7) g-r color in magnitudes. (8) Quasar classification: BAL QSO: Broad Absorption Line Quasar; Mini–BAL: Mini Broad Absorption Line Quasar, radio-loud (RL) and radio-intermediate (RI). Pν is power per unit frequency at 1.4 GHz in units of erg s−1Hz−1
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