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Table 1.

Summary of the void properties for a few example voids.

Equatorial sky coordinates Redshift Radius r Position x

Void α δ dc Void z range r ¯ $ \bar{r} $ x ¯ $ \bar{x} $ y ¯ $ \bar{y} $ z ¯ $ \bar{z} $
ID [hms] [° ] [h−1 Mpc] Match [kms−1] [h−1 Mpc] [h−1 Mpc] [h−1 Mpc] [h−1 Mpc]
10 18h05m −16.2 38.8 Local 500 − 7300 33.9 ± 3.0 341.3 ± 4.9 303.2 ± 3.4 329.7 ± 3.5
75 00h52m 43.9 33.0 Local 1500 − 5100 18.0 ± 2.0 363.7 ± 3.6 345.8 ± 2.1 363.4 ± 3.7
83 17h26m −10.9 96.0 NLV 8300 − 11 100 14.0 ± 2.6 326.7 ± 2.6 247.2 ± 2.3 322.4 ± 2.5
45 12h48m 12.9 56.1 Coma 3700 − 7500 19.0 ± 2.8 287.0 ± 4.1 329.2 ± 2.6 353.0 ± 3.1
88 14h51m 39.4 138.6 Boötes 10 000 − 18 100 39.5 ± 2.9 261.9 ± 10.7 267.7 ± 10.0 428.5 ± 9.3
15 23h48m 16.6 95.3 Pisces 7500 − 11 700 20.9 ± 3.1 431.8 ± 4.7 335.6 ± 5.6 367.7 ± 2.9
57 11h01m −29.4 65.8 Hydra 3800 − 9400 27.9 ± 3.0 285.1 ± 4.0 355.2 ± 6.1 308.2 ± 2.6
28 10h59m 2.8 43.6 Leo 2300 − 6400 20.2 ± 2.0 298.4 ± 4.0 351.9 ± 4.2 342.6 ± 3.0

Notes. The first 4 columns represent the coordinates of the center in the sky, in terms of equatorial coordinates and distance. The fourth column mentions the name of the matches we find in the literature, often corresponding to the constellation located in the direction of the void. NLV indicates the northern Local Void of Einasto et al. (1994). A more extended discussion of this comparison is presented in Section 5. Column 5 represents the redshift range from the nearest to the farther edge of the void along the line of sight, assuming the effective radius as isotropic size. Columns 6–9 represent summary properties of the posterior distributions for the effective radius and the center position, using the mean and standard deviation. In our cartesian coordinates system the observer is located at [340.5, 340.5, 340.5]h−1 Mpc, with the xy plane corresponding to the equatorial plane, and the z ̂ $ \hat{z} $ axis pointing to the equatorial north pole. The full table with all 100 voids of the catalog can be found in Appendix C.

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