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

Open Access

Table 5.

Same as Table 4, but for the case of overmassive stars.

Phase	N	N_{lone pri}	N_pri	N_sec	N $_{lone pri}^{\det}$ $_{\mathrm{lone~pri}}^{\mathrm{det}}$	N $_{lone pri}^{\det}$ $_{\mathrm{lone~pri}}^{\mathrm{det}}$ /N^det	N^det
MS	41	6	20	15	0	0.00000	7528
HG	12	4	8	0	1	0.00031	3262
RGB	57	53	4	0	45	0.00212	21 227
CHeB	236	236	0	0	226	0.01262	17 906
EAGB	22	22	0	0	22	0.00935	2354

Notes. There are no overmassive primary or secondary stars, i.e., still residing in a binary system, with detectable oscillations; therefore, their respective columns have not been included in the table.

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