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Table 2.

Blazhko star statistics for K2 fields.

C## M eA/A q0 q2 q1 q12
1 14 0.00081 0.214 0.429 0.357 0.786
2 57 0.00055 0.035 0.579 0.386 0.965
3 124 0.00048 0.000 0.387 0.613 1.000
4 38 0.00093 0.211 0.368 0.421 0.789
5 72 0.00102 0.264 0.292 0.444 0.736
6 123 0.00043 0.081 0.350 0.569 0.919
7 246 0.00114 0.183 0.451 0.366 0.817
8 45 0.00042 0.089 0.289 0.622 0.911
10 117 0.00053 0.214 0.274 0.513 0.786
11 122 0.00034 0.090 0.393 0.516 0.910
12 72 0.00046 0.097 0.431 0.472 0.903
13 31 0.00084 0.129 0.290 0.581 0.871

HQ : 660 0.00045 0.089 0.376 0.535 0.911
LQ : 401 0.00106 0.197 0.401 0.401 0.803
All: 1061 0.00068 0.130 0.385 0.484 0.870

Notes. C## is the campaign number; M is number of targets; ⟨eA/A⟩ is the average of the relative amplitude errors (Eq. (2)); q0, q2, q1, q12, respectively, are the fractions of the class 0, 2, 1, and 1 + 2 objects relative to M. The last three lines summarize the results for the high-quality fields (HQ, including C02, 03, 06, 08, 10, 11, and 12) and for the low-quality fields (LQ, including C01, 04, 05, 07, and 13). The relative amplitude errors in these lines are the averages of the campaign values weighted by M.

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