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Table 6.

Stellar velocity dispersion measured from the mock HARMONI observations of representative host galaxies of AGNs at three redshifts around cosmic noon.

Z = 0.76
Z = 1.50
Z = 2.30
Object Host S/N V* σ* S/N V* σ* S/N V* σ*
V luminosity (km s−1) (km s−1) (km s−1) (km s−1) (km s−1) (km s−1)
HSIM 389 3 158 ± 1 327 4 161 ± 1 327 0 163 ± 1
Lenticular 1012L 111 26 147 ± 3 78 16 142 ± 3 39 8 173 ± 6
(NGC 809) 1011L 51 25 152 ± 7 10 33 139 ± 16 4
1010L 6 3 < 1

HSIM 360 −39 147 ± 1 301 −39 147 ± 0 300 −38 147 ± 0
Spiral 1012L 123 −13 152 ± 2 74 −19 144 ± 3 42 −16 153 ± 11
(PGC 055442) 1011L 59 −22 147 ± 6 10 17 152 ± 20 3
1010L 7 < 1 < 1

HSIM 84 209 133 ± 9 91 201 132 ± 7 90 198 122 ± 5
Interaction 1012L 72 236 145 ± 12 48 238 133 ± 12 23 218 197 ± 33
(NGC 7119A) 1011L 41 244 144 ± 19 8 186 121 ± 38 2
1010L 5 < 1 < 1

Notes. HSIM corresponds to the HSIMInput data cube for the host scaled to 1011Lv, ⊙ in each case. The same results are obtained for the other two host luminosities. As a reference, Table A.1 lists the stellar velocity dispersion for the nearby galaxies taken as model hosts of AGNs at around cosmic noon.

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