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Table 4.

Luminosity properties of the objects described by Capak et al. (2015).

ID log(LUV/L) SFR (M yr−1) log (LX/L)
HZ1 11.21 24 10.31 8.19
HZ2 11.15 25 10.26 8.20
HZ3 11.08 18 10.21 8.10
HZ4 11.28 51 10.36 8.38
HZ5a 11.45 <3 10.82b <7.59
HZ5a <10.37 <3 <9.66 <7.59
HZ6 11.47 49 10.50 8.35
HZ6a 11.11 10.23
HZ6b 11.0 10.15
HZ6c 11.81 10.00
HZ7 11.05 21 10.19 8.11
HZ8 11.04 18 10.18 8.06
HZ8W 10.57 6 9.82 7.76
HZ9 10.95 67 10.11 8.46
HZ10c 11.14 169 10.25 8.72
HZ10Wc 10.23 9.54

Notes. The expected X-ray luminosities in the observer-frame soft band have been estimated by adopting a bolometric correction to the UV luminosity of 5.2 (Runnoe et al. 2012b).

(a)

No [C II] redshift measurement available (Capak et al. 2015), photometric redshift is used.

(b)

Luminosity in the [0.5–2] keV energy range observed in the C-COSMOS field.

(c)

These objects fall outside the C-COSMOS field.

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