Table 4.
APOLLO results for all LC candidates.
EPIC ID | νmax, FliPer | log gFliPer | log gEPIC | νmax, APOLLO | ln(Oosc, noise) | log gAPOLLO |
---|---|---|---|---|---|---|
[μHz] | [dex] | [dex] | [μHz] | [dex] | ||
204330922 | 105 | 2.0 | 2.3(9) | 109(5) | −20(16) | 2.94(10) |
205152548 | 149 | 2.2 | 2.4(4) | 151(7) | −4.09(23) | 3.09(10) |
204222295 | 150 | 2.2 | 2.4(6) | 177(14) | −77.26(23) | 3.16(11) |
204447221 | 185 | 2.3 | 2.1(5) | 225(16) | 6.55(22) | 3.26(11) |
205375290 | 219 | 3.4 | 3.2(1.5) | 242(10) | 9.07(25) | 3.30(10) |
205188906 | 322 | 2.5 | 3.2(7) | – | – | – |
204854345 | 554 | 2.7 | 2.5(7) | – | – | – |
203756781 | 572 | 2.8 | 2.6(4) | – | – | – |
205359167 | 983 | 3.0 | 2.7(3) | – | – | – |
205179845 | 2212 | 3.3 | 4.3(1.1) | – | – | – |
204121833 | 2295 | 3.4 | 4.1(9) | – | – | – |
204933717 | 2295 | 3.4 | 4.1(9) | – | – | – |
205078547 | 2560 | 3.4 | 4.1(1.4) | – | – | – |
Notes. The first three columns show the values for νmax and log g from FliPer, as well as log g from the EPIC catalogue by Huber et al. (2016). To compute νmax, APOLLO, log gAPOLLO and Oosc, noise we take the mean over the 5 successive runs of the APOLLO pipeline. The Bayes factor Oosc, noise indicates a significant result, if it exceeds a value of ln(Oosc, noise) > 5 (see Table 1).
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