Table 6.
Radio loudness.
| Source | mz | S2500 Å | S4400 Å | S5 GHz | R2500 Å | R4400 Å |
|---|---|---|---|---|---|---|
| (mag) | (mJy) | (mJy) | (mJy) | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
| J0131−0321 | (c)18.08 | 0.046 | 0.061 |
 |
 |
 |
| J0741+2520 | (c)18.44 | 0.033 | 0.043 |
 |
 |
 |
| J0836+0054 | (c, 1)18.83 | 0.022 | 0.029 |
 |
 |
 |
| J0913+5919 | (c)20.81 | 0.0037 | 0.0049 |
 |
 |
 |
| J1034+2033 | (c)19.70 | 0.010 | 0.014 |
 |
 |
 |
| J1146+4037 | (c)19.30 | 0.015 | 0.020 |
 |
 |
 |
| J1427+3312 | (c, 1)18.87 | 0.021 | 0.027 |
 |
 |
 |
| J1614+4640 | (c)19.71 | 0.010 | 0.013 |
 |
 |
 |
| J2228+0110 | (b, 1)22.28 | 0.00089 | 0.0012 |
 |
 |
 |
| J2245+0024 | (a)21.72 | 0.0016 | 0.0021 |
 |
 |
 |
Notes. Column 1: source name. Column 2: z-band AB magnitude. Columns 3−4: rest-frame 2500 Å and 4400 Å flux density, which are calculated assuming a UV power law Sν ∝ ν−0.5 with z-band photometry data. Column 5: rest-frame 5 GHz flux density predicted from our spectral fit. Columns 6−7: radio loudness. (1)z-band magnitude is contaminated by the strong Lyα line emission.
References. (a)Sharp et al. (2001); (b)Zeimann et al. (2011); (c)SDSS.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.