Table 4.
Comparison of host-galaxy-based redshift estimates to spectroscopically measured redshifts.
| (1) | (2) | (3) | (4) | (5) |
|---|---|---|---|---|
| Target | zphot | ref | zspec | ref |
| RGBJ0115+253 | 0.35 ± 0.05 | 2 | 0.376 | 3 |
| RGBJ0202+088 | 0.55 ± 0.05 | 2 | 0.629 | 10 |
| RGBJ0227+020 | 0.45 ± 0.05 | 2 | 0.458 | 4 |
| RGBJ0250+172 | 0.25 ± 0.05 | 2 | 0.243 | 3 |
| RGBJ0505+042 | 0.35 ± 0.05 | 2 | 0.424 | 11 |
| PKS0735+178 | 0.45 ± 0.06 | 6 | 0.424 | 7 |
| RGBJ0757+099 | 0.30 ± 0.05 | 2 | 0.266 | 3 |
| RGBJ1415+485 | 0.50 ± 0.05 | 2 | 0.496 | 5 |
| 3FHLJ0045.3+2127 | 0.34 ± 0.07 | 1 | 0.4253 | 8 |
| 3FHLJ0148.2+5201 | 0.38 ± 0.07 | 1 | 0.437 | 8 |
| 3FHLJ0905.5+1357 | 0.50 ± 0.09 | 1 | 0.644 ( * ) | 8 |
| 3FHLJ2031.0+1936 | 0.39 ± 0.08 | 1 | 0.3665 | 9 |
| 3FHLJ2245.9+1545 | 0.44 ± 0.09 | 1 | 0.5966 | 9 |
Notes. The upper part lists earlier imaging results, whereas the lower part refers to the results presented in this paper.
( * )See Sect. 6.1 for details about the redshift values.
(1) This work, (2) Nilsson et al. (2003), (3) La Mura et al. (2022), (4) Sbarufatti et al. (2005b), (5) SDSS DR3, (6) Nilsson et al. (2012), (7) Mishra et al. (2018), (8) Paiano et al. (2020), (9) Kasai et al. (2023), (10) Shaw et al. (2012) (11) Pita et al. (2014).
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