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Table 2

Data of superclusters.

(1) (2) (3) (4) (5) (6)

ID(long) ID Dist . L tot D peak ID(E01)

239+027+0091 1 264 1809 22.2
227+006+0078 7 233 1675 17.0 154
184+003+0077 19 231 2919 15.0 111
167+040+0078 24 225 751 14.6 95
202-001+0084 27 256 5163 14.0 126
173+014+0082 54 241 2064 12.4 111
230+027+0070 99 215 2874 11.5 158
229+006+0102 103 302 1004 11.0 160
135+038+0094 124 281 548 10.5 249
152-000+0096 126 285 1001 10.1 82
203+059+0072 143 211 753 10.1 133
172+054+0071 211 207 1618 9.2 109
216+016+0051 349 159 284 8.5 138
227+007+0045 352 135 379 8.7 154
151+054+0047 782 139 465 6.8
226+007+0090 1311 272 95 5.4

Notes.The columns are as follows: 1: Long ID of a supercluster AAA+BBB+ZZZZ, where AAA is RA, +/BBB is Dec (in degrees), and ZZZZ is 1000z (see Liivamägi et al. 2012, for details); 2: ID of a supercluster from the SDSS DR8 superclusters catalogue; 3: the distance of a supercluster, in h-1 Mpc; 4: the total weighted luminosity of galaxies in the supercluster, Ltot, in 1010h-2L; 5: the luminosity density value at the density maximum (density contrast), dpeak, in units of the mean luminosity density (Liivamägi et al. 2012); 6: ID(E01): the supercluster ID in the catalogue by Einasto et al. (2001). SCl 160 – the Hercules supercluster, SCl 111 and SCl 126 – superclusters of the Sloan Great Wall, SCl 158 – the Corona Borealis supercluster, SCl 138 – the Bootes supercluster, SCl 109 – the Ursa Major supercluster.

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