Table 2
Continuation of Table 1 with candidates from the extended sample.
| ID | RA and Dec | Redshift | line ID | NB | NB−Y | NB−J | Em.line flux | Eq. width | Ref. |
|
|
|||||||||
| (2000.0) | spectroscpic | mag (AUTO) | mag (ISO) | mag (ISO) | [10-17 erg/s/cm2] | Å | |||
|
|
|||||||||
| ELG00 | 03:32:18.57 −27:42:29.50 | 0.6045 | Hα | 22.46 ± 0.01 | −0.10 ± 0.01 | −0.55 ± 0.02 | 5.07 ± 0.05 | 69.6 ± 0.7 | (*) |
| x01 | 03:32:13.24 −27:42:40.03 | 0.6072 | Hα | 18.88 ± 0.01 | −0.36 ± 0.01 | −0.35 ± 0.01 | 227.56 ± 0.21 | 152.8 ± 0.1 | (1) |
| x02 | 03:32:23.40 −27:43:16.58 | 0.615 | Hα | 19.72 ± 0.01 | −0.47 ± 0.01 | −0.29 ± 0.01 | 98.15 ± 0.16 | 135.4 ± 0.2 | (2) |
| x03 | 03:32:41.83 −27:40:42.31 | 0.6162 | Hα | 23.35 ± 0.02 | −1.29 ± 0.04 | −1.78 ± 0.13 | 6.50 ± 0.16 | 721.0 ± 17.8 | (1) |
| x04 | 03:32:38.59 −27:46:31.36 | 0.625 | Hα | 20.87 ± 0.01 | −0.31 ± 0.01 | −0.27 ± 0.01 | 25.03 ± 0.13 | 83.4 ± 0.4 | (3) |
| x05 | 03:32:31.50 −27:41:58.04 | 0.620 | Hα | 23.32 ± 0.02 | −0.32 ± 0.02 | −0.27 ± 0.03 | 2.48 ± 0.05 | 77.0 ± 1.6 | (1) |
| x06 | 03:32:45.65 −27:44:05.80 | 0.6206 | Hα | 20.15 ± 0.01 | −0.41 ± 0.01 | −0.39 ± 0.01 | 63.40 ± 0.17 | 127.7 ± 0.3 | (1) |
| x07 | 03:32:28.01 −27:43:57.44 | 0.6207 | Hα | 21.93 ± 0.01 | −0.53 ± 0.01 | −0.78 ± 0.03 | 12.70 ± 0.16 | 133.4 ± 1.7 | (4) |
| x08 | 03:32:40.79 −27:46:15.70 | 0.6218 | Hα | 19.57 ± 0.01 | −0.36 ± 0.01 | −0.31 ± 0.01 | 85.02 ± 0.20 | 86.6 ± 0.2 | (1) |
| x09 | 03:32:46.75 −27:46:24.02 | 0.6250 | Hα | 24.86 ± 0.06 | −0.78 ± 0.06 | −1.12 ± 0.16 | 0.98 ± 0.07 | 169.8 ± 11.5 | (5) |
| x10 | 03:32:22.25 −27:49:01.47 | 1.109 | [Oiii] | 22.98 ± 0.02 | −0.19 ± 0.02 | −0.22 ± 0.03 | 2.09 ± 0.04 | 41.3 ± 0.8 | (6) |
| x11 | 03:32:27.66 −27:45:05.77 | 1.110 | [Oiii] | 23.02 ± 0.02 | −0.22 ± 0.02 | −0.34 ± 0.04 | 3.55 ± 0.09 | 86.8 ± 2.2 | (6) |
| x12 | 03:32:26.77 −27:45:30.63 | 1.122 | [Oiii] | 22.97 ± 0.02 | −0.69 ± 0.02 | −1.00 ± 0.06 | 7.11 ± 0.17 | 290.4 ± 6.8 | (6) |
| x13 | 03:32:18.81 −27:49:08.59 | 1.128 | [Oiii] | 23.19 ± 0.02 | −0.46 ± 0.02 | −0.91 ± 0.05 | 4.66 ± 0.10 | 177.2 ± 3.7 | (7) |
| x14 | 03:32:49.83 −27:46:58.30 | 1.174 | Hβ | 24.70 ± 0.06 | −1.05 ± 0.08 | −1.33 ± 0.21 | 1.44 ± 0.09 | 293.3 ± 17.8 | (1) |
| x15 | 03:32:17.11 −27:42:20.95 | 1.749 | [Neiii] | 24.52 ± 0.05 | −0.47 ± 0.05 | −0.65 ± 0.10 | 0.51 ± 0.03 | 41.2 ± 2.2 | (8) |
| x16 | 03:32:38.80 −27:47:14.82 | 1.836 | [Oii] | 22.67 ± 0.02 | −0.65 ± 0.02 | −0.08 ± 0.02 | 8.17 ± 0.16 | 209.6 ± 4.0 | (9) |
| x17 | 03:32:18.43 −27:42:51.95 | 1.846 | [Oii] | 25.08 ± 0.09 | −0.53 ± 0.09 | −0.18 ± 0.13 | 0.56 ± 0.05 | 93.5 ± 9.2 | (8) |
| x18 | 03:32:36.69 −27:46:48.48 | 1.86 | [Oii] | 24.60 ± 0.07 | −0.47 ± 0.06 | −0.17 ± 0.09 | 0.91 ± 0.07 | 101.8 ± 7.9 | (10) |
Notes. Column 1: ID number, Col. 2: coordinates of the objects. Redshift and line IDs are listed in third and fourth columns respectively. Column 5 lists narrow-band magnitudes and magnitude errors. Columns 6 and 7 present colors and color errors for Y and J filters respectively. And final three columns are emission-line fluxes, observed frame equivalent widths, and references to the literature where we obtain spectroscopic redshift.
Reference. (*) This work; (1) Balestra et al. (2010); (2) Vanzella et al. (2005); (3) Szokoly et al. (2004); (4) Le Fèvre et al. (2004); (5)Xia et al. (2011); (6) Vanzella et al. (2006); (7) Villforth et al. (2012); (8) Straughn et al. (2011); (9) Guo et al. (2012); (10) Trump et al. (2011).
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