Table B.1.
Confirmed interlopers of the F200W dropout selectiona
| ID | R.A. | Dec | zspec | F356W | zhigh | zlow | χhigh2 | χlow2 | Type |
|---|---|---|---|---|---|---|---|---|---|
| deg. | deg. | AB | |||||||
| A2744_27713 | 3.522866 | -30.351297 | - | 28.56 ± 0.07 | 18.7 | 2.9 | 0.46 | 3.28 | 1 |
| CEERS_15937 | 214.944272 | 52.835847 | 4.91 | 27.15 ± 0.09 | 17.2 | 4.6 | 0.27 | 0.84 | 2 |
| CEERS_81406b | 214.914542 | 52.943021 | 4.91 | 26.52 ± 0.03 | 16.3 | 4.6 | 0.94 | 3.90 | 3 |
| COSMOS_31168 | 150.180936 | 2.260756 | 2.29 | 27.67 ± 0.16 | 16.2 | 4.0 | 2.85 | 1.31 | 3 |
| COSMOS_35731 | 150.133571 | 2.271020 | 3.66 | 28.54 ± 0.09 | 15.9 | 2.8 | 1.07 | 0.88 | 3 |
| COSMOS_76919 | 150.184553 | 2.353510 | 5.18 | 28.71 ± 0.18 | 16.1 | 4.0 | 1.76 | 0.74 | 3 |
| UDS_56824 | 34.454893 | -5.215586 | 6.56 | 26.51 ± 0.12 | 19.8 | 4.2 | 1.45 | 1.93 | 3 |
a) ID, coordinates and F356W magnitudes from M24. The best-fit photometric redshift solutions were obtained with ZPHOT at z > 10 (zhigh) and z < 10 (zlow). The last column report the classification discussed in Sect. 3.2 and 4.2 (1=transient; 2=quiescent; 3=dusty star-forming).
b) Object CEERS-93316 from Arrabal Haro et al. (2023b).
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