Table 4
Derived parameters for our LBG samples.
| ID | Median z | Rest 2–10 keVa | Rest 2–10 keV errb | SFR | SFR errb | M ∗ | M∗ err | sSFR | sSFR errb |
| log (W) | log (W) | M⊙ yr-1 | M⊙ yr-1 | 1010 M⊙ | 1010 M⊙ | Gyr-1 | Gyr-1 | ||
|
|
|||||||||
| ref-lowZ | 0.68 | 33.20 | 32.44 | 3.19 | 0.55 | 6.73 | 1.61 | 0.04 | 0.01 |
| BZ-UV | 1.33 | 33.79 | 32.86 | 11.62 | 1.45 | 3.35 | 0.67 | 0.37 | 0.11 |
| Spec-U1 | 2.67 | 34.11 | 33.45 | 25.86 | 5.40 | 1.16 | 0.29 | 2.23 | 0.21 |
| Spec-U2 | 3.33 | 34.17 | 33.52 | 29.68 | 6.63 | 1.09 | 0.28 | 2.71 | 1.11 |
| Spec-B1 | 3.70 | 34.67 | 34.16 | 93.86 | 29.04 | 1.09 | 0.21 | 8.66 | 2.06 |
| Spec-B2 | 4.16 | 34.56 | u.l. | 72.86 | u.l. | 1.15 | 0.31 | 6.32 | u.l. |
Notes. For the convenience of the reader, we note that 1 W = 107 erg s-1.
Assuming a power-law X-ray spectrum with a photon index Γ = 2.0 typical for LBGs (Laird et al. 2006). This factor is adopted throughout the stacking literature, see e.g. Nandra et al. (2002) or Lehmer et al. (2005).
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