Table 3
Number of independent frequencies detected after cleaning for nonlinear interactions and spurious frequencies (NI); number of frequency combinations found and removed (NC), and number of spurious frequencies found and removed (NS).
| NI | NC | NS | A–D test | |||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Star ID | A | L | G | A | L | G | A | L | G | AG | AL | LG |
| HD 50844 | 1189 | 1124 | 1001 | 237 | 214 | 168 | 320 | 319 | 320 | 1.9 × 10−5 | 7.4 × 10−6 | 4.6 × 10−10 |
| HD 174936 | 520 | 550 | 348 | 82 | 81 | 68 | 268 | 284 | 164 | 2.3 × 10−3 | 4.4 × 10−2 | 2.1 × 10−4 |
| HD 174966 | 364 | 583 | 152 | 42 | 21 | 8 | 239 | 412 | 136 | 3.4 × 10−15 | 7.1 × 10−12 | 1.4 × 10−22 |
| HD 181555 | 1782 | 1786 | 2054 | 171 | 211 | 196 | 151 | 157 | 250 | 3.5 × 10−30 | 5.5 × 10−11 | 3.1 × 10−47 |
| HD 49434 | 1232 | 1284 | 2243 | 287 | 161 | 308 | 93 | 96 | 199 | 2.9 × 10−48 | 4.7 × 10−10 | 7.8 × 10−41 |
| HD 172189 | 1360 | 1275 | 1790 | 114 | 284 | 158 | 150 | 177 | 151 | 3.3 × 10−40 | 9.6 × 10−29 | 1.1 × 10−26 |
| HD 174532 | 516 | 532 | 405 | 107 | 132 | 89 | 328 | 377 | 284 | 1.5 × 10−9 | 2.9 × 10−8 | 3.3 × 10−16 |
| HD 174589 | 237 | 246 | 116 | 58 | 80 | 35 | 208 | 260 | 100 | 5.9 × 10−25 | 4.3 × 10−5 | 4.1 × 10−34 |
| HD 51722 | 1461 | 2913 | 1379 | 210 | 53 | 178 | 179 | 284 | 193 | 5.9 × 10−23 | 5.3 × 10−34 | 3.1 × 10−35 |
| HD 51359 | 1692 | 1681 | 2634 | 144 | 244 | 175 | 174 | 229 | 306 | 5.7 × 10−28 | 9.1 × 10−10 | 6.3 × 10−29 |
| HD 50870 | 2041 | 3294 | 2150 | 204 | 219 | 207 | 239 | 290 | 260 | 3.3 × 10−21 | 6.3 × 10−28 | 2.0 × 10−18 |
| HD 170699 | 2878 | 2993 | 2042 | 238 | 150 | 198 | 326 | 392 | 310 | 1.4 × 10−12 | 1.1 × 10−1 | 1.5 × 10−10 |
| GSC 00144–03031 | 2971 | 2174 | 1735 | 73 | 304 | 157 | 444 | 429 | 285 | 6.2 × 10−12 | 8.8 × 10−11 | 1.5 × 10−5 |
| HD 41641 | 2017 | 2833 | 2301 | 182 | 249 | 238 | 351 | 419 | 389 | 1.6 × 10−17 | 7.7 × 10−14 | 6.1 × 10−4 |
| HD 48784 | 183 | 171 | 141 | 28 | 32 | 43 | 253 | 222 | 139 | 2.1 × 10−3 | 3.0 × 10−1 | 8.3 × 10−3 |
Notes. Columns (A, L, G) correspond, respectively, to the frequencies detected in ARMA interpolated, linearly interpolated, and gapped light curves. Thelast three columns represent the Anderson–Darling (AD) test applied to the histogram densities of each (A, L, G) case compared by pairs: A with G, A with L, and L with G, respectively. These values correspond to the p-value of the AD test. The null hypothesis is that compared samples arose from a common distribution.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.