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Table 2

Summarised characteristics of our detections.

Target SVLBI SVLBI/SVLA rms K-corr.aL1.4 GHz Restoring beam TB z Linear scale Host νYSN νSNR
(μJy) (μJy/beam) (× 1023 W/Hz) (mas2) (× 104 K) (pc) typee (SN yr-1) (SN yr-1)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)

RQ26 157 0.49 52 ... ... ... 1.59b ... ... ...
RL106 155 ± 29 0.43 ± 0.08 17 6.6 ± 1.2 ~ 67 × 38 2.7 ± 0.5 1.06c 544 × 308 P ~126 ~11
RL728 109 0.33 36 ... ... ... 1.08b ... SB ... ...
RQ174 125 0.42 42 ... ... ... 2.85c ... MS ... ...
RQ851 110 ± 26 0.50 ± 0.12 19 9.7 ± 2.3 ~ 62 × 44 2.5 ± 0.6 1.35d 521 × 370 MS ~163 ~15
RQ76 186 ± 36 0.69 ± 0.14 23 17.2 ± 3.3 ~ 67 × 43 4.0 ± 0.8 1.38b 564 × 362 SB ~290 ~26

Notes.

(a)

Rest-frame 1.4 GHz luminosities were obtained by using measured 1.45 GHz spectral indices, based on data from Hales et al. (2014) and Huynh et al. (2012). For RQ851 and RQ76, 5 GHz information is lacking, and we adopted the value of 0.75 (e.g., Kukula et al. 1998);

(b)

spectroscopic, Silverman et al. (2010);

(c)

photometric, Rafferty et al. (2011);

(d)

photometric, Taylor et al. (2009);

(e)

from Bonzini et al. (2015): P = Passive; SB = starbust galaxy; MS = main sequence galaxy.

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