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Table 7.

Properties of the megaparsec-scale overdensities around the radio sources.

Galaxy ID zspec (RA)ov (Dec)ov θov zov Significance Nselected PPM w
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
DES-RG 399 0.388439 40.58809994 −0.5746418 92.1″ 0.34 ± 0.06 2.6σ 0.2 6 (1.3) 100″ 175″
486 kpc 528 kpc 923 kpc
DES-RG 708 0.60573 41.34062917 −0.54419315 9.3″ 0.61 ± 0.05 6.0σ 0.2 17 (2.3) 150″ 125″
62 kpc 1007 kpc 839 kpc
COSMOS-FRI 16 0.9687 150.54213359 2.27617522 35.5″ 0.93 ± 0.06 3.1σ 0.2 121 (93.0) 100″ 107″
282 kpc 795 kpc 850 kpc
150.50776446 2.25025075 124.1″ 1.06 ± 0.06 5.5σ 0.2 247 (198.9) 145″ 155″
986 kpc 1152 kpc 1232 kpc
COSMOS-FRI 31 0.9123 149.63013031 1.9426736 102.6″ 0.96 ± 0.05 2.3σ 0.2 34 (24.5) 112″ 106″
802 kpc 876 kpc 829 kpc
COSMOS-FRI 70 2.625 150.64167779 2.29597309 82″ 2.65 ± 0.04 2.8σ 0.15 7 (1.6) 87″ 88″
655 kpc 694 kpc 702 kpc

Notes. (1)–(2) Galaxy ID and spectroscopic redshift; (3)–(4) J2000 projected space coordinates of the overdensity peak as found by the wavelet transform; (5) projected separation between the coordinates in Cols. (3)–(4) and those of the radio source; overdensity redshift (6) and significance (7) as found by the PPM; photometric redshift bin (8) and number of sources (9) selected by the PPM to detect the overdensity, while between parentheses there is corresponding average number of sources in the survey within the same redshift bin and overdensity area; (10)–(11) radius of the overdensity as found by the PPM and by the wavelet transform. Columns (5),(10),(11) are reported in units of both arcseconds and kiloparsecs (physical).

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