Table 1.
Properties of the four confirmed HzRGs.
| Name | z | F(Lyα) | Width | EW | g | r | i | Ks | F76 | F1.4 | αr |
|---|---|---|---|---|---|---|---|---|---|---|---|
| NVSS J021439–002359 | 3.642 | 1.85±0.30 | 1530±250 | > 150 | 26.41 | 24.85 | 24.79 | – | 0.09 | 0.005 | –1.28 |
| NVSS J220526–291029 | 3.448 | 2.48±0.23 | 1070± 90 | > 290 | 24.71 | 23.35 | 23.13 | 19.99 | 1.39 | 0.137 | –0.80 |
| NVSS J221708–325449 | 3.799 | 2.56±0.30 | 900± 80 | > 130 | 25.27 | 23.85 | 23.87 | 21.45 | 0.82 | 0.064 | < − 1.3 |
| NVSS J231647–344233 | 3.272 | 0.82±0.16 | 1190±190 | 440±210 | 21.88 | 20.31 | 19.89 | 18.59 | 2.26 | 0.278 | –0.72 |
Notes. Properties of the four confirmed HzRGs: NVSS name, estimated redshift of the source, Lyα flux in 10−16 erg s−1 cm−2 units, line width (in km s−1), observed EW (in Å), and the magnitudes in the g, r, i, and Ks bands. We also report the radio flux (in Jy) at 76 MHz from the GLEAM catalog (except for NVSS J021439-002359, for which we list the flux density at 150 MHz), the flux density at 1.4 GHz from the National Radio Astronomy Observatory Very Large Array Sky Survey (NVSS; Condon et al. 1998), and the radio spectral index αr.
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