Table 1.
Open in new tab

A summary of some basic quantities associated with void catalogues obtained in Ref-L0100N1504 and DM-L0100N1504 (top and bottom tables, respectively) at z = 0.0 The first column shows the type of tracer that was used for void identification: subhaloes selected by their stellar mass, subhaloes selected by their total mass or the mass field (individual particles). The remaining columns, from left to right, show the total number of voids, maximum, minimum and mean void radius for each sample.

Void sampleNvoidrmaxrminrmean
(Mpc)(Mpc)(Mpc)
Ref-L0100N1504
40 per cent overlap
Mstel subhalo selection70924.34.97.0
Mtot subhalo selection70821.44.96.7
Mass field769518.31.42.5
30 per cent overlap
Mstel subhalo selection48524.34.97.1
Mtot subhalo selection47021.44.96.8
Mass field568018.31.42.5
20 per cent overlap
Mstel subhalo selection34124.34.97.1
Mtot subhalo selection33021.44.96.9
Mass field425518.31.42.5
DM-L0100N1504
40 per cent overlap
Mtot subhalo selection69321.04.96.7
Mass field953618.61.42.4
30 per cent overlap
Mtot subhalo selection46621.04.96.8
Mass field678518.61.42.4
20 per cent overlap
Mtot subhalo selection34621.04.96.8
Mass field502118.61.42.4
Void sampleNvoidrmaxrminrmean
(Mpc)(Mpc)(Mpc)
Ref-L0100N1504
40 per cent overlap
Mstel subhalo selection70924.34.97.0
Mtot subhalo selection70821.44.96.7
Mass field769518.31.42.5
30 per cent overlap
Mstel subhalo selection48524.34.97.1
Mtot subhalo selection47021.44.96.8
Mass field568018.31.42.5
20 per cent overlap
Mstel subhalo selection34124.34.97.1
Mtot subhalo selection33021.44.96.9
Mass field425518.31.42.5
DM-L0100N1504
40 per cent overlap
Mtot subhalo selection69321.04.96.7
Mass field953618.61.42.4
30 per cent overlap
Mtot subhalo selection46621.04.96.8
Mass field678518.61.42.4
20 per cent overlap
Mtot subhalo selection34621.04.96.8
Mass field502118.61.42.4
Table 1.
Open in new tab

A summary of some basic quantities associated with void catalogues obtained in Ref-L0100N1504 and DM-L0100N1504 (top and bottom tables, respectively) at z = 0.0 The first column shows the type of tracer that was used for void identification: subhaloes selected by their stellar mass, subhaloes selected by their total mass or the mass field (individual particles). The remaining columns, from left to right, show the total number of voids, maximum, minimum and mean void radius for each sample.

Void sampleNvoidrmaxrminrmean
(Mpc)(Mpc)(Mpc)
Ref-L0100N1504
40 per cent overlap
Mstel subhalo selection70924.34.97.0
Mtot subhalo selection70821.44.96.7
Mass field769518.31.42.5
30 per cent overlap
Mstel subhalo selection48524.34.97.1
Mtot subhalo selection47021.44.96.8
Mass field568018.31.42.5
20 per cent overlap
Mstel subhalo selection34124.34.97.1
Mtot subhalo selection33021.44.96.9
Mass field425518.31.42.5
DM-L0100N1504
40 per cent overlap
Mtot subhalo selection69321.04.96.7
Mass field953618.61.42.4
30 per cent overlap
Mtot subhalo selection46621.04.96.8
Mass field678518.61.42.4
20 per cent overlap
Mtot subhalo selection34621.04.96.8
Mass field502118.61.42.4
Void sampleNvoidrmaxrminrmean
(Mpc)(Mpc)(Mpc)
Ref-L0100N1504
40 per cent overlap
Mstel subhalo selection70924.34.97.0
Mtot subhalo selection70821.44.96.7
Mass field769518.31.42.5
30 per cent overlap
Mstel subhalo selection48524.34.97.1
Mtot subhalo selection47021.44.96.8
Mass field568018.31.42.5
20 per cent overlap
Mstel subhalo selection34124.34.97.1
Mtot subhalo selection33021.44.96.9
Mass field425518.31.42.5
DM-L0100N1504
40 per cent overlap
Mtot subhalo selection69321.04.96.7
Mass field953618.61.42.4
30 per cent overlap
Mtot subhalo selection46621.04.96.8
Mass field678518.61.42.4
20 per cent overlap
Mtot subhalo selection34621.04.96.8
Mass field502118.61.42.4
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