Table E.2.
Number of KNe and KNe + GRB detected by Rubin, operating in synergy with ET + 2 CE for the two observational strategies 1ep and 2ep and following up events with sky localisation Ω90<1 deg2.
| APR4 | BLh | ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| Ω90 | Transient | Uniform | Gaussian | Uniform | Gaussian | ||||||
| [deg2] | Followed | Detected | Followed | Detected | Followed | Detected | Followed | Detected | |||
| 1ep/2ep | 1ep/2ep | 1ep/2ep | 1ep/2ep | ||||||||
| α = 0.5 | ET-Δ + 2CE |
1 | KN | 1609 (3.2%) | 430/227 | 976 (1.9%) | 362/206 | 1503 (3.0%) | 350/196 | 953 (1.9%) | 529/293 |
| KN+GRB | 528/299 | 424/260 | 448/261 | 582/349 | |||||||
| ET-2L + 2CE |
1 | KN | 1830 (3.6%) | 481/251 | 1149 (2.3%) | 426/235 | 1677 (3.3%) | 393/214 | 1104 (2.2%) | 586/337 | |
| KN+GRB | 605/341 | 501/300 | 502/283 | 652/403 | |||||||
| α = 1.0 | ET-Δ + 2CE |
1 | KN | 8162 (16.2%) | 2266/1266 | 4956 (9.8%) | 2086/1195 | 7398 (14.7%) | 1868/1024 | 4824 (9.6%) | 2848/1673 |
| KN+GRB | 2595/1476 | 2301/1359 | 2192/1231 | 3017/1845 | |||||||
| ET-2L + 2CE |
1 | KN | 8818 (17.5%) | 2401/1322 | 5502 (10.9%) | 2176/1250 | 8147 (16.2%) | 1954/1087 | 5367 (10.6%) | 3006/1724 | |
| KN+GRB | 2735/1533 | 2402/1416 | 2301/1306 | 3191/1910 | |||||||
Notes. Both the triangular and 2L-shaped ET configurations are considered. The analysis is performed using different EOSs (APR4 or BLh), NS mass distributions (uniform or Gaussian), and α values (0.5 and 1.0). For each scenario, we report the total number of followed events (within Rubin's footprint), the corresponding telescope time required for follow-up (expressed as a percentage below the number of followed events), and the number of detected events. All listed data refer to 10 years of observations.
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