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Table C.1

Mass, kinematical parameters (weighted by the luminosity in the V band and by the stellar content of the particles), and magnitudes (at high redshift and at present day) for the S0 remnants resulting from GalMer major and minor merger simulations.

Luminosity weighted Mass weighted
Model log (M⋆) V circ σ 0 V rot,max V circ σ 0 V rot,max MB(z = 0.8) MK(z = 0.8) MB(z = 0) MK(z = 0)
[M⊙] [km s-1] [km s-1] [km s-1] [km s-1] [km s-1] [km s-1] [mag] [mag] [mag] [mag]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
gE0 11.20 ... 205.2 ± 4.2 23 ± 9 1 ... 206.0 ± 4.9 12 ± 4 −20.9 −25.1 ... ...
gS0 11.05 240 ± 2 103.2 ± 0.6 250 ± 0.3 244 ± 3 103.8 ± 0.5 251 ± 0.4 −20.5 −24.7 ... ...
gSa 11.05 252 ± 3 100.0 ± 0.1 259 ± 0.5 247 ± 2 97.9 ± 0.1 257 ± 1 −21.7 −25.2 ... ...
gSb 10.75 194 ±2 77.7 ± 0.8 197 ± 0.4 192 ± 2 78.8 ± 0.8 194 ± 0.4 −21.6 −24.6 ... ...
gSd 10.75 174 ± 2 50.5 ± 0.7 171 ± 0.4 174 ± 2 51.2 ± 0.6 169 ± 0.4 −22.3 −24.8 ... ...
1 gE0gSao1† 11.44 261 ± 9 243.4 ± 3.4 154 ± 6 261 ± 9 249.9 ± 0.9 149 ± 5 −21.3 −26.2 −20.2 −25.4
2 gE0gSao16 11.44 ... 240.8 ± 3.1 53 ± 3 ... 247.6 ± 2.9 44 ± 3 −21.3 −26.2 −20.1 −25.4
3 gE0gSao44 11.44 ... 247.2 ± 3.4 83 ± 6 ... 251.2 ± 3.1 94 ± 5 −21.3 −26.2 −20.1 −25.4
4 gE0gSao5† 11.44 285 ± 10 226.0 ± 3.0 145 ± 6 282 ± 10 240.2 ± 0.9 140 ± 5 −21.3 −26.2 −20.2 −25.4
5 gE0gSbo44 11.34 ... 220.2 ± 3.4 94 ± 6 ... 222.6 ± 2.8 89 ± 5 −21.1 −25.9 −20.0 −25.2
6 gE0gSbo5 11.34 154 ± 4 208.4 ± 3.6 124 ± 4 168 ± 6 209.5 ± 3.3 123 ± 4 −21.1 −25.9 −20.0 −25.2
7 gE0gSdo16 11.36 ... 209.3 ± 3.1 127 ± 2 ... 223.9 ± 2.3 93 ± 7 −21.4 −26.0 −20.1 −25.3
8 gE0gSdo44 11.36 ... 204.9 ± 2.9 125 ± 3 ... 216.5 ± 2.7 100 ± 3 −21.3 −26.0 −20.2 −25.3
9 gE0gSdo5† 11.36 169 ± 5 208.4 ± 3.8 163 ± 5 169 ± 4 214.3 ± 3.6 143 ± 5 −21.3 −26.0 −20.2 −25.2
10 gS0dE0o100† 11.11 196 ± 5 205.0 ± 0.7 158 ± 2 196 ± 5 205.8 ± 0.7 158 ± 2 −20.4 −25.3 −19.4 −24.7
11 gS0dE0o101 11.11 182 ± 2 209.6 ± 0.7 176 ± 2 180 ± 2 210.7 ± 0.7 176 ± 2 −20.4 −25.3 −19.4 −24.7
12 gS0dE0o102 11.11 191 ± 3 183.4 ± 0.8 157 ± 2 193 ± 3 184.0 ± 0.7 156 ± 2 −20.4 −25.3 −19.4 −24.7
13 gS0dE0o103† 11.11 232 ± 9 208.1 ± 0.7 159 ± 2 234 ± 9 209.2 ± 0.7 157 ± 2 −20.4 −25.3 −19.4 −24.7
14 gS0dE0o104† 11.11 225 ± 8 209.6 ± 0.7 155 ± 2 226 ± 8 210.6 ± 0.7 155 ± 2 −20.4 −25.3 −19.4 −24.7
15 gS0dE0o105† 11.11 234 ± 9 210.9 ± 0.7 162 ± 2 233 ± 9 211.9 ± 0.7 163 ± 2 −20.4 −25.3 −19.4 −24.7
16 gS0dE0o106 11.11 182 ± 2 193.2 ± 0.8 144 ± 3 202 ± 6 193.7 ± 0.7 142 ± 2 −20.4 −25.3 −19.4 −24.7
17 gS0dE0o109 11.11 195 ± 3 171.2 ± 0.8 176 ± 2 196 ± 3 171.6 ± 0.7 175 ± 2 −20.4 −25.3 −19.4 −24.7
18 gS0dE0o110† 11.11 208 ± 7 191.0 ± 0.8 157 ± 2 208 ± 7 191.9 ± 0.7 157 ± 2 −20.4 −25.3 −19.4 −24.7
19 gS0dE0o111 11.11 192 ± 3 193.7 ± 0.8 167 ± 2 202 ± 4 195.2 ± 0.7 167 ± 2 −20.4 −25.3 −19.4 −24.7
20 gS0dE0o113† 11.11 207 ± 5 212.7 ± 0.7 175 ± 2 207 ± 5 214.0 ± 0.7 176 ± 2 −20.4 −25.3 −19.4 −24.7
21 gS0dE0o115† 11.11 200 ± 4 183.3 ± 0.8 158 ± 2 199 ± 4 183.8 ± 0.7 158 ± 2 −20.4 −25.3 −19.4 −24.7
22 gS0dE0o117† 11.11 200 ± 4 194.2 ± 0.7 163 ± 2 200 ± 4 194.8 ± 0.7 164 ± 2 −20.4 −25.3 −19.4 −24.7
23 gS0dE0o98† 11.11 199 ± 5 189.9 ± 0.8 164 ± 2 200 ± 5 190.6 ± 0.7 165 ± 2 −20.4 −25.3 −19.4 −24.7
24 gS0dE0o99 11.11 204 ± 3 203.1 ± 0.7 170 ± 2 204 ± 6 204.1 ± 0.7 172 ± 2 −20.4 −25.3 −19.4 −24.7
25 gS0dS0o100 11.09 191 ± 2 173.0 ± 0.8 164 ± 2 196 ± 3 173.3 ± 0.7 165 ± 2 −20.3 −25.2 −19.3 −24.6
26 gS0dS0o101† 11.09 194 ± 4 188.4 ± 0.8 167 ± 2 195 ± 4 188.8 ± 0.7 166 ± 2 −20.3 −25.2 −19.3 −24.6
27 gS0dS0o102 11.09 194 ± 3 198.1 ± 0.7 163 ± 2 196 ± 3 199.3 ± 0.7 162 ± 2 −20.3 −25.2 −19.3 −24.6
28 gS0dS0o103† 11.09 228 ± 8 174.1 ± 0.8 175 ± 2 229 ± 7 174.1 ± 0.7 174 ± 2 −20.3 −25.2 −19.3 −24.6
29 gS0dS0o105 11.09 209 ± 3 205.9 ± 0.7 181 ± 2 209 ± 3 206.7 ± 0.7 183 ± 2 −20.3 −25.2 −19.3 −24.6
30 gS0dS0o97 11.09 202 ± 3 186.9 ± 0.7 173 ± 1 205 ± 3 187.9 ± 0.7 174 ± 1 −20.3 −25.2 −19.3 −24.6
31 gS0dS0o98 11.09 193 ± 3 167.6 ± 0.7 171 ± 2 195 ± 3 168.1 ± 0.7 171 ± 1 −20.3 −25.2 −19.3 −24.6
32 gS0dS0o99 11.09 201 ± 3 176.2 ± 0.7 168 ± 2 203 ± 3 177.0 ± 0.7 167 ± 2 −20.3 −25.2 −19.3 −24.6
33 gS0dSao10 11.09 208 ± 3 206.0 ± 0.7 171 ± 2 208 ± 3 209.3 ± 0.6 175 ± 2 −20.3 −25.3 −19.3 −24.6
34 gS0dSao103† 11.09 216 ± 6 205.6 ± 0.7 168 ± 2 214 ± 6 208.8 ± 0.7 170 ± 2 −20.3 −25.3 −19.3 −24.6
35 gS0dSao105† 11.09 225 ± 8 194.8 ± 0.7 170 ± 2 225 ± 7 197.4 ± 0.7 173 ± 2 −20.3 −25.3 −19.3 −24.6
36 gS0dSao106† 11.09 224 ± 8 207.2 ± 0.7 166 ± 2 220 ± 8 209.9 ± 0.6 170 ± 2 −20.3 −25.3 −19.4 −24.6
37 gS0dSbo106† 11.07 230 ± 7 178.1 ± 0.8 196 ± 1 245 ± 5 178.0 ± 0.7 198 ± 1 −20.3 −25.2 −19.3 −24.6
38 gS0dSdo100 11.07 201 ± 3 169.6 ± 0.6 176 ± 1 197 ± 3 174.7 ± 0.6 175 ± 1 −20.3 −25.2 −19.4 −24.6
39 gSagSao1† 11.37 242 ± 9 221.3 ± 2.4 170 ± 3 240 ± 8 225.2 ± 2.2 165 ± 3 −21.3 −26.0 −19.9 −25.2
40 gSagSao5† 11.38 282 ± 12 214.8 ± 2.6 188 ± 4 281 ± 12 224.9 ± 0.8 184 ± 4 −21.3 −26.1 −19.9 −25.2
41 gSagSao9† 11.38 238 ± 17 192.7 ± 2.1 206 ± 3 239 ± 17 208.1 ± 0.7 209 ± 3 −21.2 −26.0 −19.9 −25.2
42 gSagSbo1† 11.26 263 ± 11 201.7 ± 2.2 157 ± 3 258 ± 11 209.0 ± 2.0 154 ± 3 −21.1 −25.8 −19.8 −24.9
43 gSagSbo2 11.26 ... 201.8 ± 2.3 144 ± 3 ... 209.9 ± 0.7 132 ± 3 −21.1 −25.8 −19.8 −24.9
44 gSagSbo21† 11.26 250 ± 9 136.0 ± 4.9 138 ± 3 250 ± 8 132.7 ± 4.9 122 ± 3 −21.1 −25.7 −19.7 −24.9
45 gSagSbo22† 11.26 242 ± 6 198.1 ± 2.2 143 ± 3 ... 220.6 ± 0.7 129 ± 3 −21.1 −25.7 −19.7 −24.9
46 gSagSbo5† 11.26 232 ± 15 194.1 ± 2.2 173 ± 4 254 ± 10 209.7 ± 0.7 168 ± 3 −21.1 −25.8 −19.7 −24.9
47 gSagSbo9† 11.26 204 ± 5 189.2 ± 0.6 183 ± 3 204 ± 5 207.2 ± 0.6 184 ± 3 −21.1 −25.8 −19.7 −24.9
48 gSagSdo2† 11.27 222 ± 11 187.4 ± 2.4 177 ± 3 194 ± 21 196.1 ± 1.9 170 ± 3 −21.4 −25.9 −20.0 −25.0
49 gSagSdo42† 11.27 248 ± 10 179.0 ± 2.3 182 ± 3 229 ± 14 193.7 ± 1.2 173 ± 5 −21.2 −25.8 −19.9 −24.9
50 gSagSdo5† 11.27 249 ± 9 178.9 ± 1.8 179 ± 3 249 ± 10 192.9 ± 1.5 172 ± 3 −21.3 −25.9 −20.0 −25.0
51 gSagSdo9† 11.28 190 ± 11 187.8 ± 2.1 180 ± 3 215 ± 6 205.4 ± 0.6 176 ± 3 −21.3 −25.9 −19.9 −24.9
52 gSbgSbo22 11.10 ... 171.2 ± 3.1 27 ± 1 ... 184.7 ± 0.6 27 ± 2 −20.8 −25.4 −19.6 −24.5
53 gSbgSbo72† 11.11 151 ± 4 217.9 ± 2.4 91 ± 2 ... 221.9 ± 2.2 76 ± 2 −20.8 −25.4 −19.5 −24.5
54 gSbgSbo9† 11.10 203 ± 5 171.5 ± 2.0 148 ± 3 187 ± 7 177.5 ± 0.5 142 ± 3 −20.8 −25.4 −19.6 −24.5
55 gSbgSdo14† 11.12 148 ± 4 141.4 ± 2.3 85 ± 4 143 ± 4 152.6 ± 2.2 80 ± 4 −21.0 −25.4 −19.7 −24.5
56 gSbgSdo17 11.12 ... 177.8 ± 2.5 57 ± 3 ... 190.5 ± 2.3 54 ± 9 −21.0 −25.4 −19.7 −24.6
57 gSbgSdo18 11.13 ... 177.8 ± 2.5 57 ± 3 ... 190.5 ± 2.3 54 ± 9 −21.0 −25.5 −19.7 −24.6
58 gSbgSdo19 11.12 ... 118.7 ± 8.2 25 ± 2 ... 119.9 ± 8.1 20 ± 2 −21.0 −25.4 −19.8 −24.5
59 gSbgSdo41† 11.12 214 ± 8 134.5 ± 2.0 134 ± 3 211 ± 7 145.9 ± 1.9 121 ± 3 −21.0 −25.4 −19.8 −24.6
60 gSbgSdo5† 11.12 245 ± 9 168.4 ± 2.9 163 ± 4 246 ± 9 173.9 ± 1.7 152 ± 4 −21.1 −25.5 −19.7 −24.6
61 gSbgSdo69† 11.12 205 ± 7 129.3 ± 1.8 150 ± 3 203 ± 7 135.8 ± 1.6 140 ± 3 −21.0 −25.4 −19.7 −24.5
62 gSbgSdo70† 11.12 163 ± 4 154.1 ± 1.8 145 ± 2 175 ± 4 164.7 ± 1.7 136 ± 3 −21.0 −25.4 −19.8 −24.6
63 gSbgSdo9† 11.12 199 ± 14 157.1 ± 1.7 170 ± 4 225 ± 9 169.9 ± 1.7 164 ± 4 −21.1 −25.5 −19.8 −24.6
64 gSdgSdo17 11.14 ... 154.6 ± 4.3 28 ± 10 ... 165.4 ± 3.1 24 ± 4 −21.3 −25.6 −19.9 −24.6
65 gSdgSdo2 11.14 ... 176.1 ± 4.1 137 ± 2 ... 181.6 ± 3.3 118 ± 2 −21.4 −25.7 −20.0 −24.6
66 gSdgSdo42† 11.14 184 ± 12 152.3 ± 2.3 144 ± 2 198 ± 7 166.0 ± 2.1 123 ± 2 −21.3 −25.6 −20.0 −24.6
67 gSdgSdo5† 11.14 150 ± 10 150.5 ± 2.3 154 ± 2 184 ± 5 163.1 ± 2.2 134 ± 2 −21.4 −25.6 −20.0 −24.7
68 gSdgSdo69† 11.14 225 ± 9 120.2 ± 2.0 138 ± 2 223 ± 9 126.9 ± 1.7 127 ± 3 −21.2 −25.5 −19.9 −24.6
69 gSdgSdo71 11.14 ... 139.9 ± 2.3 98 ± 5 ... 139.9 ± 1.5 95 ± 4 −21.3 −25.6 −20.0 −24.6
70 gSdgSdo74 11.15 ... 192.7 ± 0.4 42 ± 5 ... 198.4 ± 0.4 39 ± 8 −21.3 −25.6 −19.9 −24.6
71 gSdgSdo9† 11.15 228 ± 10 151.4 ± 0.4 160 ± 2 229 ± 9 162.9 ± 0.4 138 ± 2 −21.4 −25.6 −20.0 −24.6

Notes. Columns: (1) Number ID. (2) Code g[type1]g[type2]o[orbit] of the experiment generating an S0 remnant as explained in Sect. 3.2. (3) Logarithm of the stellar mass of the remnant at the last moment of the simulation. (4, 5, 6) Circular velocity, central velocity dispersion, and maximum rotational velocity of the data weighted by the luminosity in the V band of the stellar content of the remnants, respectively. (7, 8, 9) Circular velocity, central velocity dispersion, and maximum rotational velocity for the values obtained weighting the data by the stellar mass of the particles in the remnant. (10) Total absolute magnitude in the Johnson-Cousin B band at z = 0.8. (11) Total absolute magnitude in the K band at z = 0.8. (12) Total absolute magnitude in the Johnson-Cousin B band at z = 0. (13) Total absolute magnitude in the K band at z = 0. The magnitudes are in the Vega system and have been corrected for dust extinction (see Sect. 3.3).

(†)

The circular velocity of these S0-like remnants can only be considered as an upper limit (see Sect. 3.4.2 for the explanation).

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