Table A.1.
Void counts in nine equi-spaced bins in redshift, measured in the redshift-space mock galaxy catalogue, provided as a reference for future forecast analyses.
z range | shell volume [(h−1 Gpc)3] | MGS [h−1 Mpc] | all voids |
voids after cleaning |
||||
---|---|---|---|---|---|---|---|---|
R > MGS | > 2 MGS | Reff > MGS | > 2 MGS | |||||
0.9 − 1.0 | 1.308 | 10.28 | 8928 | 6032 | 4845 | 726 | ||
1.0 − 1.1 | 1.427 | 11.02 | 8987 | 6637 | 5253 | 840 | ||
1.1 − 1.2 | 1.531 | 11.74 | 7735 | 5824 | 4690 | 699 | ||
1.2 − 1.3 | 1.622 | 12.63 | 7167 | 5237 | 4140 | 500 | ||
1.3 − 1.4 | 1.700 | 13.51 | 6575 | 4756 | 3703 | 321 | ||
1.4 − 1.5 | 1.766 | 14.45 | 5636 | 4078 | 3152 | 249 | ||
1.5 − 1.6 | 1.821 | 15.45 | 5132 | 3624 | 2719 | 160 | ||
1.6 − 1.7 | 1.867 | 16.48 | 4389 | 3049 | 2286 | 94 | ||
1.7 − 1.8 | 1.904 | 17.63 | 2248 | 934 | 851 | 4 | ||
0.9 − 1.8 | 14.95 | 13.69 | 56 797 | 40 171 | 31 639 | 3593 |
Notes. The first column represents the minimum and the maximum redshift values for each bin, while the second and the third columns provide the volume in units of (h−1 Gpc)3 corresponding to each shell of the sky octant, and the MGS, respectively. The next two columns show the number of voids identified by the VIDE void finder, selected with an effective radius greater than 1 and 2 times the MGS, respectively. In the last two columns we provide the void number counts obtained after the cleaning procedure, to be modelled using the void size function theory. The latter are reported with the same radius selections as described before. In the last row we show the total shells’ volume, the mean MGS and the total void counts corresponding to the entire range of redshifts.
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