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Table 2.
Emission properties of ESDLAs from our X-shooter observing programme.
| Quasar | zESDLA | Line luminosity (1040 erg s−1) | ρ | ||
|---|---|---|---|---|---|
| Lyα | [O III]λ5007 | Hα | (kpc) | ||
| J0017+1307 | 2.326 | <27.2 | <43.9 | <127.7 | … |
| J0025+1145 | 2.304 | <16.3 | 178 ± 21 | 198 ± 61 | 1.9 ± 0.1 |
| J1143+1420 | 2.323 | <30.2 | 120 ± 15 | <351 | 0.6 ± 0.3 |
| J1258+1212 | 2.444 | <11.9 | <249 | <334 | … |
| J1349+0448 | 2.482 | <9.2 | <92 | <402 | … |
| J1411+1229 | 2.545 | <12 | <63 | <274 | … |
| J1513+0352 | 2.464 | 9.6 ± 3.5 | <69 | <131 | 1.4 ± 0.9 |
| J2140−0321 | 2.339 | <12 | <130 | <76 | … |
| J2232+1242 | 2.230 | <8.7 | <137 | <72 | … |
| J2246+1328 | 2.215 | <7.4 | <36 | <88 | … |
| J2322+0033 | 2.477 | <14 | <46 | <317 | … |
Notes. All measurements are from this work, except J1513+0352 (from Ranjan et al. 2018). The upper limits correspond to the mean detection limit in the spatial area covered by the slit (see text).
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