Table D.1.
Identification of the spectroscopically confirmed LAEs that were predicted by our models. The source compilation used was Khostovan et al. (2025). For each source, we present their Cosmos ID, the COSMOS2020 right ascension and declination in degrees, the spectroscopic redshift from the corresponding survey, the average prediction score attributed by our models and the corresponding reference of the observing program.
| ID | RA | DEC | z | Prediction score | Reference |
|---|---|---|---|---|---|
| 234035 | 149.93480 | 1.63806 | 4.270 | 0.64 | Hasinger et al. (2018) |
| 364107 | 150.28945 | 1.76708 | 3.536 | 0.93 | Hasinger et al. (2018) |
| 882240 | 149.96797 | 2.25817 | 4.825 | 0.83 | Hasinger et al. (2018) |
| 1015255 | 150.34350 | 2.38053 | 4.865 | 0.66 | Hasinger et al. (2018) |
| 1063117 | 149.96235 | 2.42651 | 4.331 | 0.53 | Hasinger et al. (2018) |
| 1065656 | 149.86276 | 2.42895 | 4.252 | 0.92 | Hasinger et al. (2018) |
| 1145690 | 150.32957 | 2.50640 | 4.375 | 0.55 | Hasinger et al. (2018) |
| 1364946 | 149.90115 | 2.71935 | 4.417 | 0.75 | Hasinger et al. (2018) |
| 935357 | 150.13882 | 2.30700 | 3.002 | 0.51 | Le Fèvre et al. (2015), Tasca et al. (2017) |
| 926044 | 150.10998 | 2.29865 | 2.579 | 0.52 | Le Fèvre et al. (2015), Tasca et al. (2017) |
| 1027774 | 150.11771 | 2.39110 | 3.685 | 0.68 | Le Fèvre et al. (2015), Tasca et al. (2017) |
| 986789 | 150.17796 | 2.35369 | 2.663 | 0.76 | Le Fèvre et al. (2015), Tasca et al. (2017) |
| 1186357 | 150.19970 | 2.54533 | 3.99 | 0.80 | Le Fèvre et al. (2015), Tasca et al. (2017) |
| 1194293 | 150.17779 | 2.55310 | 2.931 | 0.86 | Le Fèvre et al. (2015), Tasca et al. (2017) |
| 1189474 | 150.11301 | 2.54828 | 2.475 | 0.75 | Le Fèvre et al. (2015), Tasca et al. (2017) |
| 960881 | 150.12266 | 2.33115 | 3.100 | 0.83 | Schmidt et al. (2021) |
| 855981 | 150.11998 | 2.23466 | 5.245 | 0.52 | Schmidt et al. (2021) |
| 851264 | 150.16004 | 2.23055 | 3.362 | 0.50 | Schmidt et al. (2021) |
| 840426 | 150.10451 | 2.22100 | 5.306 | 0.77 | Schmidt et al. (2021) |
| 835220 | 150.16006 | 2.21626 | 3.009 | 0.69 | Schmidt et al. (2021) |
| 833340 | 150.12719 | 2.21475 | 3.393 | 0.96 | Schmidt et al. (2021) |
| 830930 | 150.17496 | 2.21229 | 2.973 | 0.53 | Schmidt et al. (2021) |
| 830219 | 150.09378 | 2.21195 | 3.393 | 0.80 | Schmidt et al. (2021) |
| 828510 | 150.10382 | 2.21038 | 3.244 | 0.94 | Schmidt et al. (2021) |
| 820571 | 150.12293 | 2.20322 | 4.97 | 0.86 | Schmidt et al. (2021) |
| 841033 | 150.09003 | 2.22157 | 3.247 | 0.81 | Rosani et al. (2020) |
| 862699 | 150.15868 | 2.24061 | 3.613 | 0.81 | Rosani et al. (2020) |
| 963145 | 150.11921 | 2.33318 | 3.006 | 0.63 | Rosani et al. (2020) |
| 297187 | 149.64846 | 1.70356 | 5.755 | 0.56 | Ning et al. (2020) |
| 897108 | 150.10767 | 2.27187 | 5.858 | 0.77 | Pentericci et al. (2018) |
| 709082 | 149.91040 | 2.10059 | 2.602 | 0.98 | Lee et al. (2018), Horowitz et al. (2022) |
| 746299 | 149.91977 | 2.13525 | 2.414 | 0.73 | Lee et al. (2018), Horowitz et al. (2022) |
| 746990 | 149.89142 | 2.13569 | 2.885 | 0.99 | Lee et al. (2018), Horowitz et al. (2022) |
| 772090 | 150.36777 | 2.15830 | 2.614 | 0.87 | Lee et al. (2018), Horowitz et al. (2022) |
| 779372 | 150.12211 | 2.16507 | 2.986 | 0.61 | Lee et al. (2018), Horowitz et al. (2022) |
| 780988 | 150.26258 | 2.16598 | 2.601 | 0.77 | Lee et al. (2018), Horowitz et al. (2022) |
| 818249 | 150.20273 | 2.20032 | 2.628 | 0.99 | Lee et al. (2018), Horowitz et al. (2022) |
| 831491 | 150.03077 | 2.21253 | 2.710 | 0.98 | Lee et al. (2018), Horowitz et al. (2022) |
| 1005589 | 150.22114 | 2.37094 | 2.517 | 0.71 | Lee et al. (2018), Horowitz et al. (2022) |
| 1014763 | 149.98645 | 2.37882 | 2.545 | 0.96 | Lee et al. (2018), Horowitz et al. (2022) |
| 1072458 | 149.89117 | 2.43519 | 2.682 | 0.70 | Lee et al. (2018), Horowitz et al. (2022) |
| 1087513 | 149.95876 | 2.45026 | 2.627 | 0.99 | Lee et al. (2018), Horowitz et al. (2022) |
| 1107108 | 150.03117 | 2.46885 | 2.540 | 0.83 | Lee et al. (2018), Horowitz et al. (2022) |
| 1115349 | 150.33797 | 2.47537 | 2.403 | 0.67 | Lee et al. (2018), Horowitz et al. (2022) |
| 1127921 | 150.14896 | 2.48828 | 2.380 | 0.60 | Lee et al. (2018), Horowitz et al. (2022) |
| 1001949 | 150.12686 | 2.36819 | 2.675 | 0.99 | The HETDEX collaboration (2023) |
| 882398 | 150.19893 | 2.25778 | 2.611 | 0.99 | The HETDEX collaboration (2023) |
| 876293 | 150.27823 | 2.25241 | 2.611 | 0.99 | The HETDEX collaboration (2023) |
| 902799 | 150.24821 | 2.27721 | 2.880 | 0.97 | The HETDEX collaboration (2023) |
| 861537 | 150.22581 | 2.23847 | 2.947 | 0.95 | The HETDEX collaboration (2023) |
| 919305 | 150.26890 | 2.29190 | 2.763 | 0.92 | The HETDEX collaboration (2023) |
| 920040 | 150.11345 | 2.29203 | 2.289 | 0.91 | The HETDEX collaboration (2023) |
| 852094 | 150.11932 | 2.23086 | 2.886 | 0.88 | The HETDEX collaboration (2023) |
| 1000124 | 150.26582 | 2.36609 | 2.552 | 0.86 | The HETDEX collaboration (2023) |
| 869170 | 150.24103 | 2.24515 | 3.444 | 0.84 | The HETDEX collaboration (2023) |
| 846881 | 150.20089 | 2.22575 | 2.481 | 0.84 | The HETDEX collaboration (2023) |
| 904304 | 150.11306 | 2.27872 | 2.138 | 0.80 | The HETDEX collaboration (2023) |
| 875173 | 150.09854 | 2.25180 | 3.173 | 0.78 | The HETDEX collaboration (2023) |
| 975976 | 150.20227 | 2.34395 | 3.326 | 0.68 | The HETDEX collaboration (2023) |
| 817254 | 150.14991 | 2.19838 | 2.698 | 0.50 | The HETDEX collaboration (2023) |
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