Open Access

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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