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

Open Access

Table 8.

Overmassive stars in the case of the E06 binary prescription. See also Table 5.

Phase	N	N_{lone pri}	N_pri	N_sec	N $_{lone pri}^{\det}$ $_{\mathrm{lone~pri}}^{\mathrm{det}}$	N $_{pri}^{\det}$ $_{\mathrm{pri}}^{\mathrm{det}}$	N $_{\sec}^{\det}$ $_{\mathrm{sec}}^{\mathrm{det}}$	N $_{lone pri}^{\det}$ $_{\mathrm{lone~pri}}^{\mathrm{det}}$ /N^det	N $_{pri}^{\det}$ $_{\mathrm{pri}}^{\mathrm{det}}$ /N^det	N $_{\sec}^{\det}$ $_{\mathrm{sec}}^{\mathrm{det}}$ /N^det	N^det
MS	4288	4194	83	11	189	0	0	0.02464	0.00000	0.00000	7671
HG	540	534	6	0	69	0	0	0.02076	0.00000	0.00000	3323
RGB	777	773	3	1	508	2	1	0.02355	0.00009	0.00005	21 568
CHeB	738	738	0	0	701	0	0	0.03929	0.00000	0.00000	17 843
EAGB	103	103	0	0	103	0	0	0.04233	0.00000	0.00000	2433

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