DUETS: Setting expectations for asteroseismic binaries and binary products with synthetic populations

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Table 2.

Similar to Table 1, but limited to stars with detectable oscillations.

Phase	N^det	N $_{\sin}^{\det}$ $^{\mathrm{det}}_{\mathrm{sin}}$	N $_{lone pri}^{\det}$ $^{\mathrm{det}}_{\mathrm{lone~pri}}$	N $_{pri}^{\det}$ $^{\mathrm{det}}_{\mathrm{pri}}$	N $_{\sec}^{\det}$ $^{\mathrm{det}}_{\mathrm{sec}}$	(N $_{pri}^{\det}$ $^{\mathrm{det}}_{\mathrm{pri}}$ + N $_{\sec}^{\det}$ $^{\mathrm{det}}_{\mathrm{sec}}$ )/N^det	N $_{pri}^{seismo}$ $^{\mathrm{seismo}}_{\mathrm{pri}}$	N $_{\sec}^{seismo}$ $^{\mathrm{seismo}}_{\mathrm{sec}}$	(N $_{pri}^{seismo}$ $^{\mathrm{seismo}}_{\mathrm{pri}}$ + N $_{\sec}^{seismo}$ $^{\mathrm{seismo}}_{\mathrm{sec}}$ )/N^det
MS	7528	5381	0	2099	48	0.28520	30	33	0.00837
HG	3262	2205	1	1038	18	0.32373	7	5	0.00368
RGB	21 227	15 046	91	5952	138	0.28690	49	24	0.00344
CHeB	17 906	12 307	703	4653	243	0.27343	58	81	0.00776
EAGB	2354	1743	53	511	47	0.23704	7	8	0.00637
TP-AGB	139	119	4	16	0	0.11511	0	0	0.00000
Post-AGB	23	1	2	15	5	0.86957	0	0	0.00000
CO-WD	0	0	0	0	0	0.00000	0	0	0.00000
He-WD	0	0	0	0	0	0.00000	0	0	0.00000

Notes. Total number of stars (“N^det”), single stars (“N $_{\sin}^{\det}$ $_{\mathrm{sin}}^{\mathrm{det}}$ ”), lone primaries (“N $_{lone pri}^{\det}$ $_{\mathrm{lone~pri}}^{\mathrm{det}}$ ”), primaries (“N $_{pri}^{\det}$ $_{\mathrm{pri}}^{\mathrm{det}}$ ”) and secondaries (“N $_{\sec}^{\det}$ $_{\mathrm{sec}}^{\mathrm{det}}$ ”) with detectable oscillations. “N $_{pri}^{seismo}$ $_{\mathrm{pri}}^{\mathrm{seismo}}$ ” and “N $_{pri}^{seismo}$ $_{\mathrm{pri}}^{\mathrm{seismo}}$ ” are the number of stars in each evolutionary phase that are in asteroseismic binaries as primaries or secondaries, respectively.

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