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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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