Table 1.
Characteristics of the over-densities studied in this work.
| RA | Dec | Field | Name | N | Volume | Dark Matter Halo | AGN | Zspec | Zphot |
|---|---|---|---|---|---|---|---|---|---|
| [J2000] | [J2000] | [Mpc3] | [1012 M⊙] | ||||||
| 53.1346 | −27.6954 | CDFS | z323 | 27 | 8186 ± 614 | 0.74 [2.33, 0.13] | 0 | 3 | 24 |
| 53.1229 | −27.7404 | CDFS | z329 | 31 | 13356 ± 581 | 3.60 [8.69, 0.93] | 0 | 3 | 28 |
| 53.0137 | −27.7388 | CDFS | z343 | 10 | 281 ± 91 | 14.90 [28.60, 5.44] | 2 | 7 | 3 |
| 53.0985 | −27.8060 | CDFS | z354 | 22 | 5645 ± 871 | 0.49 [1.63, 0.07] | 0 | 4 | 18 |
| 53.1187 | −27.8596 | CDFS | z355 | 82 | 31230 ± 1974 | 28.50 [49.30, 12.10] | 5 | 8 | 74 |
| 53.0712 | −27.6921 | CDFS | z369 | 18 | 3184 ± 445 | 0.54 [1.79, 0.09] | 0 | 5 | 13 |
| 34.2602 | −5.2498 | UDS | z324 | 31 | 5527 ± 829 | 3.17 [7.81, 0.79] | 0 | 4 | 27 |
| 34.4552 | −5.2023 | UDS | z327 | 20 | 1422 ± 266 | 1.32 [3.76, 0.27] | 0 | 1 | 19 |
| 34.5203 | −5.1648 | UDS | z332 | 29 | 8015 ± 903 | 0.69 [2.17, 0.12] | 0 | 4 | 25 |
| 34.4027 | −5.1648 | UDS | z349 | 7 | 139 ± 34 | 0.13 [0.55, 0.01] | 0 | 1 | 6 |
| 34.3427 | −5.2423 | UDS | z351 | 10 | 1230 ± 131 | 0.17 [0.67, 0.21] | 0 | 0 | 10 |
| 34.5186 | −5.2356 | UDS | z365 | 11 | 994 ± 164 | 0.29 [1.07, 0.42] | 0 | 4 | 7 |
| 34.5427 | −5.2023 | UDS | z369 | 48 | 18090 ± 1940 | 0.78 [16.70, 2.45] | 0 | 5 | 43 |
| 53.0705 | −27.8685 | CDFS | G–A | 39 | 9938 ± 652 | 3.09 [7.66, 0.77] | 2 | 5 | 34 |
| 53.1132 | −27.8698 | CDFS | G–B | 25 | 2915 ± 188 | 13.60 [26.50, 4.87] | 3 | 3 | 22 |
| 53.1593 | −27.8771 | CDFS | G–C | 16 | 1803 ± 164 | 0.84 [2.57, 0.15] | 0 | 0 | 16 |
Notes. The table columns correspond to (1) right ascension and (2) declination of the highest density peak, (3) field, (4) nomenclature, (5) total number of members, (6) maximum volume given by the redshift range of the members, the uncertainty corresponds to the photometric redshift uncertainty of the VANDELS catalog, (7) dark matter halo mass, estimated from the total stellar mass of members using the calibration provided by van der Burg et al. (2014). Values in brackets indicate the lower and upper limits according to this calibration, (8) number of X-ray-detected and emission line AGN, (9) number of spectroscopic redshifts, and (10) number of photometric redshifts for the over-density members.
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