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Table 4

Supercluster candidates detected in the eFEDS field.

ID RA Dec N z l(z) Mtot C
(deg) (deg) (Mpc) (1015 M⊙)
eFEDS-SC1 133.622 +1.201 4 0.107 19.43 0.4 1
eFEDS-SC2 132.914 +0.729 6 0.195 21.39 1.2 0.77
eFEDS-SC3 135.091 +3.009 10 0.196 21.43 3.1 0.58
eFEDS-SC4 140.531 +3.925 6 0.269 24.33 2.2 0.87
eFEDS-SC5 129.959 –1.700 7 0.269 24.34 1.9 0.83
eFEDS-SC6 139.996 +2.435 5 0.282 24.86 1.8 1
eFEDS-SC7 135.390 –1.209 4 0.295 25.38 0.9 1
eFEDS-SC8 133.289 +1.397 4 0.324 26.17 1.0 0.57
eFEDS-SC9 141.682 –1.053 6 0.337 26.69 1.8 0.44
eFEDS-SC10(*) 130.690 +1.045 4 0.342 27.02 0.8 0.86
eFEDS-SC11 143.707 +0.076 4 0.344 27.13 1.3 0.72
eFEDS-SC12 143.862 +0.641 4 0.358 28.23 3.0 1
eFEDS-SC13 129.769 +2.121 5 0.359 28.35 2.3 1
eFEDS-SC14 130.666 +1.226 8 0.414 33.45 2.6 0.49
eFEDS-SC15 138.423 +3.922 4 0.456 37.49 2.3 1
eFEDS-SC16(*) 129.502 –2.060 6 0.565 47.02 4.4 0.77
eFEDS-SC17(*) 140.134 +4.198 4 0.579 49.24 2.5 0.68
eFEDS-SC18(*) 137.574 +3.182 4 0.619 58.18 2.1 0.65
eFEDS-SC19(*) 136.418 +2.489 7 0.803 65.70 5.2 0.49

Notes. We mark with an asterisk in brackets the superclusters in which for more than half of the members no spectroscopic redshifts are available. The coordinates and redshifts are the mean values of the member clusters. C is the compactness; see text for more details.

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