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Table A.3

Sculptor-type dSphs.

Run Apo Peri T iso,1 T iso,2 T iso,3
[kpc] [kpc] [Gyr] [Gyr] [Gyr]

scl103 105 35.8 12.1 9.5 6.9
scl104 105 44.6 11.9 9.1 6.3
scl105 105 53.3 11.8 8.8 5.8
scl106 105 61.9 11.7 8.5 5.2
scl107 105 70.5 11.8 8.3 4.8
scl153 150 36.2 11.7 8.0 4.3
scl154 150 45.2 11.5 7.6 3.7
scl155 150 54.1 11.4 7.3 3.2
scl156 150 62.9 11.4 7.0 2.6
scl157 150 71.7 11.4 6.8 2.1
scl203 200 36.5 11.1 6.0 1.0
scl204 200 45.5 10.9 5.7 0.4
scl205 200 54.5 10.8 5.3
scl206 200 63.5 10.8 5.0
scl207 200 72.5 10.8 4.7
scl253 250 36.6 10.4 3.9
scl254 250 45.7 10.2 3.6
scl255 250 54.8 10.1 3.2
scl256 250 63.9 10.1 2.8
scl257 250 73.0 10.0 2.6

Notes. Simulation parameters for Sculptor-like dSphs. Tiso,n is the time the dSph evolves in isolation before passing the perigalacticon n times.

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