Table 1.
Sample and archival data I.
| Source | z | S120 MHz | S147.5 MHz | S232 MHz | S325 MHz | S1.4 GHz | S1.6 GHz | S1.7 GHz | S5 GHz | S8.4 GHz | S32 GHz |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (mJy) | (mJy) | (mJy) | (mJy) | (mJy) | (mJy) | (mJy) | (mJy) | (mJy) | (mJy) | ||
| J0131−0321 | (t)5.18 ± 0.01 | – | (x,1)25.70 ± 4.70 | – | - | (w)33.69 ± 0.12 | – | (v)64.40 ± 0.30 | – | – | – |
| J0741+2520 | (k)5.194 | - | – | – | – | (w)2.97 ± 0.14 | – | – | – | – | – |
| J0836+0054 | (e)5.774 ± 0.003 | – | – | – | – | (d)1.75 ± 0.04 | (b)1.10 ± 0.03 | – | (f)0.34 ± 0.04 | – | – |
| J0913+5919 | (m)5.1224 ± 0.0001 | – | – | (h)30.00 ± 3.00 | – | (c)19.41 ± 0.12 | – | – | (d)8.10 ± 0.20 | – | – |
| J1034+2033 | (z)5.0150 ± 0.0005 | – | – | – | – | (w)3.85 ± 0.14 | – | – | – | – | – |
| J1146+4037 | (m)5.0059 ± 0.0007 | – | – | – | – | (w)12.53 ± 0.15 | (l)15.50 ± 0.80 | – | (l)8.60 ± 0.40 | – | – |
| J1427+3312 | (g)6.12 | – | – | – | (u)4.80 ± 0.80 | (j)1.78 ± 0.11 | (i)0.92 | – | (i)0.46 | (j)0.25 ± 0.02 | – |
| J1429+5447 | (p)6.1831 ± 0.0007 | (y)10.86 ± 1.55 | – | – | – | (w)2.95 ± 0.15 | (n)3.30 ± 0.06 | – | (n)0.99 ± 0.06 | – | (p)0.26 ± 0.02 |
| J1614+4640 | (z)5.3131 ± 0.0013 | – | – | – | – | (w)2.16 ± 0.14 | – | – | – | – | – |
| J2228+0110 | (q)5.95 | – | – | – | – | (o)0.31 ± 0.06 | (s)0.30 ± 0.12 | – | – | – | – |
| J2239+0030 | (r)5.09 | – | – | – | – | (o)1.22 ± 0.08 | – | – | – | – | – |
| J2245+0024 | (a)5.17 | – | – | – | – | (o)1.09 ± 0.06 | – | – | – | – | – |
Notes. Column 1: source name. Column 2: redshift. Columns 3–12: the flux density of each observing frequency.
We pulled the image containing our source from TGSS (Intema et al. 2017), and adopted CASA 2D Gaussian fit tool to calculate the flux density as well as its error. This source does not appear in the TGSS online dataset because they used a 7σ cut.
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