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Table 2.
Gaussian fits to the Lyα-like emission lines.
| Chandra window | Mg XII offset | Mg XIIFWHM | Si XIV offset | Si XIVFWHM | S XVI offset | S XVIFWHM |
|---|---|---|---|---|---|---|
| (km s−1) | (km s−1) | (km s−1) | (km s−1) | (km s−1) | (km s−1) | |
| Obs-1 | −102 ± 28 | 1302 ± 76 | −1 ± 24 | 1241 ± 77 | −4 ± 67 | 1021 ± 268 |
| Obs-2 | 136 ± 24 | 1041 ± 70 | 153 ± 16 | 1168 ± 52 | 25 ± 44 | 1005 ± 188 |
| Obs-2.A | 9 ± 21 | 869 ± 68 | −28 ± 18 | 1166 ± 57 | −85 ± 52 | 1049 ± 213 |
| Obs-2.B | 172 ± 48 | 1199 ± 130 | 213 ± 31 | 1207 ± 96 | 64 ± 86 | 1152 ± 342 |
| Obs-2.C | 664 ± 88 | 1236 ± 247 | 598 ± 44 | 950 ± 156 | 322 ± 110 | 680 ± 634 |
| GTC-2 | 384 ± 106 | 1294 ± 273 | 460 ± 56 | 889 ± 207 | 312 ± 220 | 1349 ± 776 |
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