Table 3.
Properties of our targets.
| Galaxy ID | RA | Dec | zspec | 
|
|
L1.4 GHz | Radio | Optical |
|---|---|---|---|---|---|---|---|---|
| (hh:mm:ss.sss) | (dd:mm:ss.sss) | (mJy) | (mJy) | (1032 erg s−1 Hz−1) | morphology | morphology | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| DES-RG 399 | 02:42:27.221 | −00:34:41.732 | 0.38844 ± 0.00004 | 12.54 | 12.0 | 0.59 | Unresolved | Smooth |
| DES-RG 708 | 02:45:21.751 | −00:32:29.782 | 0.60573 | 11.80 | 36.0 | 5.00 | Extended | Smooth |
| COSMOS-FRI 16 | 10:02:09.053 | +02:16:02.478 | 0.9687 ± 0.0005 | 5.70 | 4.4 | 1.86 | Unresolved | Smooth |
| COSMOS-FRI 31 | 09:58:28.598 | +01:54:58.896 | 0.9123 ± 0.0003 | 3.71 | 4.1 | 1.50 | Compact | Smooth |
| COSMOS-FRI 70 | 10:02:28.769 | +02:17:21.970 | 2.625 ± 0.003 | 3.90 | 4.5 | 19.49 | Compact | — |
Notes. (1) Galaxy name; (2)–(3) J2000 equatorial coordinates, for the sources DES-RG 399 and 708 the coordinates of the DES counterparts are reported, while those of COSMOS-FRI 16, 31, and 70 are from Castignani et al. (2014a); (4) spectroscopic redshift and uncertainty of DES-RG 399 (from the BOSS survey, Dawson et al. 2013, as found in the DR14 of SDSS), of DES-RG 708 (DES spectroscopic dataset; C. Benoist, priv. comm.), of COSMOS-FRI 16 and 31 (from MAGELLAN, Trump et al. 2007), and of COSMOS-FRI 70 (zCOSMOS-deep; M. Bolzonella, priv. comm.); (5)–(6) FIRST and NVSS flux densities; (7) rest frame 1.4 GHz luminosity density estimated using Eq. (1); (8)–(9) radio and optical morphology inferred from the images reported in Figs. 1 and 2, the morphology of COSMOS-FRI sources is from Chiaberge et al. (2009).
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