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Table 4.

Density peaks/proto-clusters/proto-groups already found in the literature.

Literature
From this work
ID Ref. z δgal σv Mtot Volume δgal Mtot Match with δgal Volume Mtote σv eMvire
(Fig. 6) (km s−1) (1014 M) cMpc3 (1014 M) this work cMpc3 (1014M) (km s−1) (1014 M)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15)
L16a 4 2.450 1.6 ± 0.9b 1568b 1.50b 0.83b [3]*
L16b 4 2.443 1.6 ± 0.9b 1568b 1.50b 0.83b [3]*
L16c 4 2.435 1.6 ± 0.9b 1568b 1.50b 0.83b [3]*
W16 5 2.506 530 ± 120 429 2.46 0.29 [5] 3.11 252 0.190 533 0.82
F16 8 2.442 9.27 ± 4.93 770 15.5/14.1d ∼10 000 1.04 4.89 [3] 3.03 805 0.598 417 0.41
D15 1 2.450 10 426 1513 1.99 0.92 [3] 3.03 805 0.598 417 0.41
Ca15 2 2.472 11c > 0.8 ± 0.3 8839 1.55 4.82 [1] 3.79 3134 2.648 731 2.16
Ch15 3 2.440 4a ∼12 000 0.53 ∼5.6 [3]*
Ch14 7 2.450 ∼23 000 0.37 ∼9.1 [3]*
D13a 6 2.476 264 87 3.12 0.07 [1]*
D13b 6 2.469 488 253 3.73 0.21 [1]*
D13c 6 2.469 239 108 4.26 0.10 [4] 3.20 720 0.552 672 1.68
D13d 6 2.463 30 26 4.08 0.02 [1]*
D13e 6 2.452 476 38 0.89 0.02 [1]*
D13f 6 2.440 526 425 2.87 0.31 [3] 3.03 805 0.598 417 0.41

Notes. (1) ID of the proto-structures, as the labels in Fig. 6. (2) References: 1- Diener et al. (2015); 2- Casey et al. (2015); 3- Chiang et al. (2015); 4- Lee et al. (2016); 5- Wang et al. (2016); 6- Diener et al. (2013); 7- Chiang et al. (2014); 8- Franck & McGaugh (2016). (3), (4), (5), and (6) are the redshift, the overdensity value, the velocity dispersion and the total halo mass, taken from the corresponding paper, when available; in some cases, the redshift is the central redshift of the used redshift slice. When necessary, total masses from the literature are converted so as to correspond to h = 0.70. Column (7) is the volume of the overdensity peaks as described in their respective papers, while (8) and (9) are the average δgal and total mass (computed with Eq. (1)) as computed in our 3D data cube in the volume quoted in Col. (7). (10) matching peak of this work (see also the discussions in Sect. 4.2); the asterisks mark the cases when the match is not one-to-one, or there is a slight mis-match between the centres, and in these cases we quote our closest peak, as discussed in Sect. 4.2. Columns from (11) to (15) are average overdensity, volume, Mtot, σv and Mvir of the matching peak in this work (see Tables 1 and 3) in the cases of a clear match.

(a)

The overdensity is computed using LAE galaxies.

(b)

The three subcomponents L16a, L16b and L16c are treated together as one single proto-cluster by Lee et al. (2016) when they compute the total mass, so the quoted number is the overall mass comprising the three components, for both the values in their paper (Col. 6) and as recovered in this work (Cols. 7, 8 and 9).

(c)

The overdensity is computed using DSFG galaxies.

(d)

The first mass is the overdensity mass, the second the virial mass.

(e)

For the sake of clarity, we omit the uncertainties, which are already reported in the previous tables.

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