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Table B.4.

Properties of low stellar mass [log(M/M) ≤ 6.0] stacked LBG candidates.

zph Sources # (a) Weight (b) log(IRX) (c) CLEAN (d) Flux (e)(f) S/N(g)
[μJy]
equal < 3.12 Natural −16 ± 27 −0.59
Taper −41 ± 36 −1.14
pbcor < 3.11 Natural −16 ± 27 −0.59
Taper −41 ± 36 −1.14
z <  4.0 8 FUV < 2.94 Natural −25 ± 34 −0.74
Taper −40 ± 44 −0.91
μ < 3.19 Natural −22 ± 30 −0.73
Taper −45 ± 38 −1.18

equal < 2.87 Natural 5 ± 43 0.12
Taper −30 ± 67 −0.45

pbcor < 2.87 Natural 5 ± 43 0.12
Taper −30 ± 67 −0.45
4.0 ≤ z <  7.0 3 FUV < 2.87 Natural −3 ± 44 −0.07
Taper −23 ± 68 −0.34
μ < 2.87 Natural 5 ± 43 0.12
Taper −30 ± 67 −0.45
equal Natural
Taper
pbcor Natural
Taper
7.0 ≤ z 0 FUV Natural
Taper
μ Natural
Taper

Notes.

(a)

When Source # is zero (0), no stacking was performed.

(b)

Weight scheme associated to each candidate, as explained in Sect. 3.2.

(c)

3-σ upper limits of weighted average for each bin (Eq. (16)).

(d)

CLEANing method used in CASA to obtain final image.

(e)

Maximum value from a box in the stacked images.

(f)

rms errors from Eq. (6).

(g)

S/N = Fluxpeak/rms.

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