Table 3
Same as Tables 1 and 2, but with different cuts on the catalogue UCBs with frequencies above 5 mHz to identify UCBs worthy follow-up analysis by EM observatories.
| Observation time | Sky localisation 10 sq. deg. |  |
 |
Eclipsing 70° < i(deg.) < 110° | Eclipsing with  |
Eclipsing with  , and well-localised |
|---|---|---|---|---|---|---|
| 1.5 | 2 | 279 | 5 | 91 | 16 | 0 |
| 3.0 | 3 | 553 | 1 | 372 | 48 | 0 |
| 6.0 | 25 | 1950 | 10 | 1027 | 275 | 4 |
| 12.0 | 441 | 4239 | 20 | 1873 | 735 | 58 |
Notes. A catalogue UCB is added to each column when at least 90% of its MCMC samples satisfy the given condition. In the first cut we state the number of UCBs that are “well-localised”, with sources contained within a sky location area of 10 deg2. In the next two columns, we have the number of UCB with positive and negative frequency derivatives. The number of eclipsing binaries is shown in Col. 5, and we further subdivide this category into the last two columns. Eclipsing with GW dominated frequency evolution, and the number of UCBs which are eclipsing and well-localised. From this final category we select a high frequency 12-month catalogue UCB, as an example of a target for follow-up EM observations and archival searches.
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