Table 5
Predicted number of Galactic solvable BH/NS-LCs with Gaia.
Binary type | Observation time | ![]() |
N1 | N2 | N3 |
---|---|---|---|---|---|
BH-LC | 5 yr | <30% | ![]() |
![]() |
![]() |
BH-LC | 5 yr | <10% | ![]() |
![]() |
![]() |
NS-LC | 5 yr | <30% | ![]() |
![]() |
![]() |
NS-LC | 5 yr | <10% | ![]() |
![]() |
![]() |
BH-LC | 10 yr | <30% | ![]() |
![]() |
– |
BH-LC | 10 yr | <10% | ![]() |
![]() |
– |
NS-LC | 10 yr | <30% | ![]() |
![]() |
– |
NS-LC | 10 yr | <10% | ![]() |
![]() |
– |
Notes. The statistical result is discussed in Sect. 4.5. Columns 1–3 list the basic information of the sample, from which we calculate [N1, N2, N3] with three different methods. N1 is our result, while N2 and N3 are for comparison. All three methods use Eq. (7) to obtain σ(mp)/mp, but different Ξ values. For N1, the Ξ is calculated from Eq. (10), while we set the Φ4(P, e, i) = 1 when we calculate the Ξ for N2. For N3, we use Eq. (9) to get the Ξ, and thus the binary period and the observation time are limited within 5 yr.
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