Open Access

Table A.1.

Complete list of binary systems generated by the MDS17 simulation.

phaselate phaseearly N None Nseismo Nseismo / N late det $ _{\mathrm{late}}^{\mathrm{det}} $ Nseismo / N early det $ _{\mathrm{early}}^{\mathrm{det}} $ Nseismo / ∑ N late det $ _{\mathrm{late}}^{\mathrm{det}} $ Nseismo/∑Nseismo
MS MS 59228 2070 30 0.19868 0.00399 0.00399 0.00057
HG MS 7620 1023 2 0.01325 0.00061 0.00027 0.00004
HG 521 9 5 0.03311 0.00153 0.00153 0.00010
RGB MS 8738 5589 1 0.00662 0.00005 0.00013 0.00002
HG 484 194 0 0.00000 0.00000 0.00000 0.00000
RGB 257 133 20 0.13245 0.00094 0.00094 0.00038
CHeB MS 4975 4581 0 0.00000 0.00000 0.00000 0.00000
HG 123 43 0 0.00000 0.00000 0.00000 0.00000
RGB 145 69 29 0.19205 0.00162 0.00137 0.00055
CHeB 65 2 53 0.35099 0.00296 0.00296 0.00101
EAGB MS 518 510 0 0.00000 0.00000 0.00000 0.00000
HG 14 13 0 0.00000 0.00000 0.00000 0.00000
RGB 12 8 3 0.01987 0.00127 0.00014 0.00006
CHeB 6 2 4 0.02649 0.00170 0.00022 0.00008
EAGB 4 0 4 0.02649 0.00170 0.00170 0.00008
TP-AGB MS 16 16 0 0.00000 0.00000 0.00000 0.00000
Post-AGB MS 20 17 0 0.00000 0.00000 0.00000 0.00000
RGB 1 1 0 0.00000 0.00000 0.00000 0.00000
CO-WD MS 3570 0 0 0.00000 0.00000 0.00000 0.00000
HG 1026 1 0 0.00000 0.00000 0.00000 0.00000
RGB 1893 13 0 0.00000 0.00000 0.00000 0.00000
CHeB 1271 30 0 0.00000 0.00000 0.00000 0.00000
EAGB 120 4 0 0.00000 0.00000 0.00000 0.00000
TP-AGB 2 0 0 0.00000 0.00000 0.00000 0.00000
Post-AGB 12 0 0 0.00000 0.00000 0.00000 0.00000
He-WD MS 5647 0 0 0.00000 0.00000 0.00000 0.00000
HG 972 2 0 0.00000 0.00000 0.00000 0.00000
RGB 973 9 0 0.00000 0.00000 0.00000 0.00000
CHeB 405 3 0 0.00000 0.00000 0.00000 0.00000
EAGB 44 0 0 0.00000 0.00000 0.00000 0.00000
NS MS 463 14 0 0.00000 0.00000 0.00000 0.00000
HG 65 9 0 0.00000 0.00000 0.00000 0.00000
RGB 107 63 0 0.00000 0.00000 0.00000 0.00000
CHeB 81 45 0 0.00000 0.00000 0.00000 0.00000
EAGB 7 6 0 0.00000 0.00000 0.00000 0.00000
Post-AGB 2 2 0 0.00000 0.00000 0.00000 0.00000
BH MS 5 0 0 0.00000 0.00000 0.00000 0.00000

Notes. Similar dataset to Table 3, but extended also to combinations of primary and secondary phases that do not result in any asteroseismic binaries. Every binary in the table has an unresolved magnitude brighter than 16 mag in Kepler’s band.

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