Table 1.
Physical properties computed with BAGPIPES of the protocluster member candidates identified behind SMACS0723.
| ID | RA | Dec | zphot | logM⋆ | SFR | Av | μ [95% C.I] |
|---|---|---|---|---|---|---|---|
| [deg] | [deg] | [M⊙] | [M⊙ yr−1] | [mag] | |||
| PC_1 | 110.823826 | −73.437880 | 6.68 |
7.79 |
3.37 |
0.35 |
1.90 [1.49–2.06] |
| PC_2 | 110.820512 | −73.436305 | 7.69 |
8.19 |
1.71 |
0.11 |
1.79 [1.44–1.92] |
| PC_3 | 110.845907 | −73.435998 | 7.76 |
7.96 |
0.72 |
0.12 |
1.73 [1.41–1.83] |
| PC_4 | 110.846149 | −73.435474 | 7.20 |
8.57 |
3.25 |
0.33 |
1.70 [1.39–1.80] |
| PC_5 | 110.847412 | −73.435129 | 8.19 |
8.50 |
3.23 |
0.19 |
1.68 [1.54–1.77] |
| PC_6⋆ | 110.844634 | −73.435054 | 7.665 | 8.59 |
3.55 |
0.15 |
1.68 [1.38–1.78] |
| PC_7⋆ | 110.834062 | −73.434509 | 7.659 | 8.95 |
15.06 |
1.02 |
1.68 [1.41–1.79] |
| PC_8 | 110.835151 | −73.429499 | 7.33 |
8.26 |
2.61 |
0.54 |
1.50 [1.29–1.57] |
Notes. All the values are not corrected for the best-fit magnification. The last column shows the magnification factor estimated by the lens model presented in Pascale et al. (2022), assuming a redshift of z = 7.66 for all objects. ⋆spectroscopically confirmed at z = 7.66. Spectroscopic redshift are indicated in italics.
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