Table 3.
Photometric redshifts estimated with LePhare and EAZY as in Weaver et al. (2022), and with LePhare using BC03 templates, for the z ≥ 7.5 candidates.
| ID | zphot |
MUV | B20/S19 | Flag(a) | zspec | |||||
|---|---|---|---|---|---|---|---|---|---|---|
| LePhare | EAZY | LePhare BC03 | ||||||||
| CLASSIC | Farmer | CLASSIC | Farmer | CLASSIC | Farmer | |||||
| All criteria satisfied (gold sample) | ||||||||||
| 234500 |
 |
 |
 |
 |
 |
 |
 |
... | ... | ... |
| 336101 |
 |
 |
 |
 |
 |
 |
 |
213/Y3 | ... | 7.306/R25 |
| 403992 |
 |
 |
 |
 |
 |
 |
 |
266 | ... | ... |
| 564423 |
 |
 |
 |
 |
 |
 |
 |
237/Y5 | ... | −/R24 NIRSpec |
| 631862 |
 |
 |
 |
 |
 |
 |
 |
... | ... | ... |
| 724872 |
 |
 |
 |
 |
 |
 |
 |
... | D | ... |
| 784810 |
 |
 |
 |
 |
 |
 |
 |
598/Y10 | ... | ... |
| 852845 |
 |
 |
 |
 |
 |
 |
 |
... | ... | NIRSpec |
| 978062 |
 |
 |
 |
 |
 |
 |
 (c) |
762/Y1 | ... | 7.675/R18 NIRSpec |
| 1055131 |
 |
 |
 |
 |
 |
 |
 |
839 | ... | ... |
| 1103149 |
 |
 |
 |
 |
 |
 |
 |
879 | ... | 7.369/R19 |
| 1151531 |
 |
 |
 |
 |
 |
 |
 (c) |
914/Y2 | ... | 7.677/R36 |
| 1212944 |
 |
 |
 |
 |
 |
 |
 |
953/Y15 | ... | ... |
| 1274544 |
 |
 |
 |
 |
 |
 |
 |
... | D | ... |
| 1352064 |
 |
 |
 |
 |
 |
 |
 |
... | 2 | ... |
| 1409328 |
 |
 |
 |
 |
 |
 |
 |
... | ... | ... |
| Blended galaxies (gold sample) | ||||||||||
| 428351 |
 |
 |
 |
 |
 |
 |
 |
301/Y4 | DB | 7.090/R27 |
| 442053 |
 |
 |
 |
 |
 |
 |
 |
... | DB | ... |
| 859061 |
 |
 |
 |
 |
 |
 |
 |
Y11 | B | ... |
| 1313521 |
 |
 |
 |
 |
 |
 |
 |
... | 2B | ... |
| Potential low-redshift galaxies (based on EAZY photometric redshift, gold sample) | ||||||||||
| 1209618 |
 |
 |
 |
 |
 |
 |
 |
Y8 | ... | ... |
| 1371152 |
 |
 |
 |
 |
 |
 |
 |
Y12 | ... | ... |
| Potential low-redshift galaxies (based on LePhare photometric redshift) | ||||||||||
| 720309 |
 |
 |
 |
 |
 |
 |
 |
... | ... | ... |
| 720309 (b) | ... |
 |
... | ... | ... |
 |
... | ... | ... | ... |
| 1356755 |
 |
 |
 |
 |
 |
 |
... | ... | ... | NIRSpec |
| Potential z < 6 dusty galaxies | ||||||||||
| 241443 |
 |
 |
 |
 |
 |
 |
 |
... | 1 | ... |
| 984164 |
 |
 |
 |
 |
 |
 |
 |
... | 2 | ... |
| 1412106 |
 |
 |
 |
 |
 |
 |
 |
... | 2 | ... |
| Potential stars | ||||||||||
| 485056 |
 |
 |
 |
 |
 |
 |
 |
356 | ... | ... |
| 545752 |
 |
 |
 |
 |
 |
 |
 |
... | 1 | ... |
| 1346929 |
 |
 |
 |
 |
 |
 |
 |
1032 | ... | ... |
| Potential local noise in HSC DR3 images | ||||||||||
| 441697 |
 |
 |
 |
 |
 |
 |
 |
... | 1 | NIRSpec |
| 1297232 |
 |
 |
 |
 |
 |
 |
 |
... | 2 | ... |
Notes. The UV absolute magnitudes are derived from a Monte Carlo sampling of the galaxy zPDF, using The Farmer and LePhare. The three last columns list identifiers from S19 and B20, flagsa and spec-z from Bouwens et al. (2022). (a)The flags are the following. 1: outside the HSC ultra-deep region, 2: outside the IRAC SPLASH region, B: blended, D: inside the UltraVISTA deep stripes. (b) LePhare photo-z computed using the UltraVISTA photometry uncontaminated by the cross-talk (see Sect. 3.4). (c)Absolute magnitudes computed using the ALMA spec-z. We report the error associated with the H-band apparent magnitude.
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