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Table 1
Sample, observing log, and S/N of the spectra.
| Object/other name | RA(2000) | Dec(2000) | Obs. date | Exp. Time | S/N at λ = | ||
| h:m:s | ° ’ ” | YY-MM-DD | [s] | 700 | 855 | 1300 | |
|
|
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| ISO−Oph023/SKS1 | 16:26:18.821 | −24:26:10.52 | 2010-08-20 | 4×750s | 0 | 4 | 61 |
| ISO−Oph030/GY5 | 16:26:21.528 | −24:26:00.96 | 2010-08-20 | 4×750s | 15 | 71 | 66 |
| ISO−Oph032/GY3 | 16:26:21.899 | −24:44:39.76 | 2010-06-01 | 4×750s | 12 | 29 | 65 |
| ISO−Oph033/GY11 | 16:26:22.269 | −24:24:07.06 | 2010-08-26 | 4×1800s | 0 | 2 | 29 |
| ISO−Oph037/LFAM3/GY21 | 16:26:23.580 | −24:24:39.50 | 2010-08-21 | 4×750s | 0 | 2 | 36 |
| ISO−Oph072/WL18 | 16:26:48.980 | −24:38:25.24 | 2010-04-06 | 4×480s | 3 | 17 | 51 |
| ISO−Oph087 | 16:26:58.639 | −24:18:34.66 | 2010-08-28 | 4×750s | 0 | 2 | 29 |
| ISO−Oph094 | 16:27:03.591 | −24:20:05.45 | 2010-08-28 | 4×750s | 0 | 1 | 10 |
| ISO−Oph102/GY204 | 16:27:06.596 | −24:41:48.84 | 2010-07-23 | 4×750s | 12 | 41 | 68 |
| ISO−Oph115/WL11/GY229 | 16:27:12.131 | −24:34:49.14 | 2010-07-30 | 4×750s | 0 | 1 | 37 |
| ISO−Oph117/WLY2-32b/GY235 | 16:27:13.823 | −24:43:31.66 | 2010-06-08 | 4×480s | 3 | 17 | 92 |
| ISO−Oph123 | 16:27:17.590 | −24:05:13.70 | 2010-08-27 | 4×750s | 58 | 74 | 83 |
| ISO−Oph160/B162737-241756 | 16:27:37.422 | −24:17:54.87 | 2010-08-27 | 4×750s | 1 | 15 | 62 |
| ISO−Oph164/GY310 | 16:27:38.631 | −24:38:39.19 | 2010-06-08 | 4×750s | 6 | 31 | 45 |
| ISO−Oph165/GY312 | 16:27:38.945 | −24:40:20.67 | 2010-06-08 | 4×750s | 0 | 1 | 27 |
| ISO−Oph176/GY350 | 16:27:46.291 | −24:31:41.19 | 2010-08-21 | 4×750s | 1 | 16 | 89 |
| ISO−Oph193/B162812-241138 | 16:28:12.720 | −24:11:35.60 | 2010-08-21 | 4×750s | 2 | 28 | 24 |
Notes. Exposure times are the same in the three X-Shooter arms (UVB, VIS, and NIR). Wavelengths for the S/N calculation are reported in nm.
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