Table 2.
Upper limits on the expected number of galaxies for JWST surveys detected in the rest-frame UV.
| Survey | Area (arcmin2) | 5σ Depth | z = 7 | z = 9 | z = 11 | z = 13 | z = 15 |
|---|---|---|---|---|---|---|---|
| CEERS | 100 | 29.2 | 54 | 3 | 3 | 2 | 2 |
| Cosmos-Web | 1929 | 28.2 | 224 | 10 | 8 | 6 | 85 |
| JADES-Deep | 46 | 30.7 | 205 | 20 | 17 | 12 | 11 |
| JADES-Medium | 190 | 29.8 | 247 | 18 | 16 | 14 | 11 |
| PRIMER | 378 | 29.5 | 319 | 20 | 18 | 15 | 13 |
Notes. The expected number of objects is calculated by integrating the UV luminosity function up to the 5σ depth of the surveys. The redshift bins encompass [z − 0.5, z + 0.5]. Shown are the upper limits, given by the 95th percentile of the distribution obtained from sampling the model UVLF at different redshifts. 5σ depth and survey areas taken from Casey et al. (2022).
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