Table 1.
F200W dropout candidates in the ASTRODEEP-JWST fields.
| ID | RA | Dec | F356W | M1500 | Re | β | zhigh | zlow | χhigh2 | χlow2 |
|---|---|---|---|---|---|---|---|---|---|---|
| deg | deg | AB | kpc | |||||||
| CEERS_17384 | 214.853243 | 52.77368 | 27.11 ± 0.08 | −21.06 | 0.317 ± 0.05 | −1.50 ± 0.33 | 17.2 | 4.7 | 0.36 | 0.90 |
| JADES-GN_9538 | 189.191052 | 62.17421 | 28.90 ± 0.13 | −19.49 | 0.227 ± 0.043 | −1.63 ± 0.40 | 16.1 | 2.8 | 0.62 | 0.64 |
| COSMOS_84213 | 150.167211 | 2.368995 | 28.14 ± 0.18 | −20.35 | 0.199 ± 0.053 | −2.03 ± 0.40 | 15.6 | 4.0 | 2.31 | 1.73 |
| COSMOS_107923 | 150.107337 | 2.428780 | 25.48 ± 0.10 | −22.68 | 0.219 ± 0.024 | −1.22 ± 0.26 | 16.3 | 3.3 | 0.59 | 0.65 |
| COSMOS_118438 | 150.196541 | 2.464192 | 27.86 ± 0.19 | −20.61 | 0.256 ± 0.077 | −2.27 ± 0.47 | 17.1 | 5.0 | 1.37 | 0.37 |
Notes. ID, coordinates and F356W magnitudes from M24. The MUV and half-light radius (Rh) were measured from the observed F277W band. The UV slope β is obtained by fitting the F277W, F356W and F444W bands. The last four columns show the best-fit solutions obtained with ZPHOT at z > 10 (zhigh) and z < 10 (zlow), and the relevant χ2 values.
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