Table 1
Counts of determined redshifts for different source extractions in the MUSE Ultra Deep (udf-10), Deep field (mosaic), and the unique objects of udf-10 + the mosaic.
| udf-10 (1′ × 1′) | mosaic (3′ × 3′) | Combineda | |||||||
| Confidence level (CONFID) | ≥3 | ≥2 | ≥1 | ≥3 | ≥2 | ≥1 | ≥3 | ≥2 | ≥1 |
|
|
|||||||||
| HST continuum selectedb | 87 | 223 | 282 | 515 | 636 | 714 | 570 | 1206 | 1414 |
| With UVUDF counterpartsb | 547 | 1133 | 1295 | ||||||
| Emission line selected | 46 | 154 | 160 | 450 | 1057 | 1163 | 467 | 1112 | 1214 |
| Emission line onlyc | 2 | 30 | 31 | 15 | 114 | 144 | 15 | 132 | 160 |
|
|
|||||||||
| Total unique objects | 89 | 253 | 313 | 562 | 1247 | 1439 | 585 | 1338 | 1574 |
Notes.
For the mosaic, the HST continuum selected galaxies to inspect are limited to F775W ≤ 27 mag (Sect. 4.2.1). The rest of the galaxies are selected by direct detection of emission lines in the data cube. Among the emission line selected galaxies, some galaxies have counterparts in the UVUDF catalog with F775W> 27 mag. They are listed in the row labeled “With UVUDF counterparts” in the table.
The objects selected by emission lines that have no counterpart in the UVUDF catalog (Rafelski et al. 2015).
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