Table A.4
Radiative parameters and other parameters of interest derived from the analysis of the K2 light curves for selected long-period eclipsing binary stars.
| EPIC | SKp | ℓ3 | ℓKp | R1∕a | R2∕a | e | ω [°] | σ [ppt] |
|---|---|---|---|---|---|---|---|---|
| 201160323 | 0.62(1) | 0.43(5) | 0.75(7) | 0.0132(4) | 0.0145(3) | 0.202(3) | 154(2) | 6.2, 4.8 |
| 201161715 | 1.4(1) | 0.01(3) | 0.18(3) | 0.0446(6) | 0.0161(6) | 0.345(4) | 23(2) | 1.4, 2.7 |
| 201246763 | 1.23(2) | 0.006(6) | 1.58(4) | 0.0165(2) | 0.0186(1) | 0.519(2) | 134.4(2) | 0.8, 2.5 |
| 201253025 | 1.00(1) | 0.27(5) | 1.0(2) | 0.071(3) | 0.071(3) | 0.045(5) | 100(1) | 3.2 |
| 1.01(1) | 0.16(5) | 0.9(2) | 0.073(3) | 0.070(3) | 0.045(5) | 100(1) | 3.5 | |
| 201379113 | 0.20(9) | =0 | 0.1(1) | 0.021(2) | 0.016(1) | 0.35(4) | 124(14) | 2.6, 0.5 |
| 201382417 | 0.210(2) | 2.8(2) | 0.055(3) | 0.0893(9) | 0.0457(6) | 0.001(1) | 150(65) | 0.4, 0.4 |
| 201408204 | 0.991(8) | 0.004(4) | 0.92(2) | 0.0543(4) | 0.0524(4) | 0.202(1) | 30.3(7) | 1.2, 1.5 |
| 201488365 | 0.9945(7) | 0.0005(8) | 0.84(1) | 0.0792(2) | 0.0726(3) | 0.0001(2) | – | 0.5, 0.4 |
| 201576812 | 0.21(4) | =0 | 0.19(6) | 0.055(4) | 0.050(7) | 0.01(2) | – | 1.9, 0.9 |
| 201648133 | 0.542(2) | 0.006(3) | 0.2563(8) | 0.02082(2) | 0.01431(2) | 0.0458(8) | 243.9(5) | 0.1, 0.3 |
| 201665500 | 0.059(2) | =0 | 0.0036(1) | 0.137(1) | 0.0339(3) | 0.002(7) | – | 2.7, 1.1 |
| 201705526 | 0.128(2) | 4.5(2) | 0.046(1) | 0.0273(2) | 0.0163(2) | 0.269(2) | 336.6(8) | 0.1, 0.1 |
| 201723461 | 0.4(4) | =0 | 0.6(5) | 0.017(7) | 0.020(5) | 0.6(2) | 152(15) | 24, 22 |
| 202674012 | 0.966(3) | 0.005(5) | 0.306(2) | 0.04596(8) | 0.0258(1) | 0.027(2) | 259.7(6) | 0.3, 0.4 |
| 202843085 | 0.970(6) | 0.015(4) | 1.30(3) | 0.0490(4) | 0.0567(3) | 0.101(1) | 144(1) | 1.0, 1.3 |
| 203361171 | 0.98(4) | 0.3(3) | 1.2(4) | 0.069(6) | 0.079(5) | 0.018(3) | 189(18) | 4.2, 3.6 |
| 203371239 | 0.94(1) | 0.05(2) | 0.73(8) | 0.0388(9) | 0.034(1) | 0.039(5) | 269.0(2) | 2.7, 7.9 |
| 203543668 | 0.30(1) | 1.4(1) | 0.137(5) | 0.0166(3) | 0.0112(2) | 0.606(4) | 139(1) | 1.3, 1.2 |
| 203610780 | 0.51(6) | 1.2(2) | 2.9(3) | 0.0173(3) | 0.0411(5) | 0.37(1) | 94.1(2) | 0.8, 1.0 |
| 203636784 | 0.195(3) | 0.05(4) | 0.041(2) | 0.0780(8) | 0.0360(5) | 0.021(6) | 89.8(5) | 2.1, 1.8 |
| 203728604 | 0.860(3) | 0.012(8) | 0.127(1) | 0.0480(1) | 0.01846(6) | 0.3072(4) | 156.5(2) | 0.2, 2.4 |
| 204407880 | 0.46(2) | 0.05(3) | 0.047(2) | 0.0412(5) | 0.0130(2) | 0.592(6) | 59.6(5) | 0.4, 1.8 |
| 204748201 | 0.063(2) | 0.16(6) | 0.0115(7) | 0.0588(8) | 0.0250(4) | 0.001(3) | – | 1.4, 1.8 |
| 204760247 | 0.389(6) | 0.06(4) | 0.167(8) | 0.0689(7) | 0.0451(9) | 0.001(3) | – | 8.7 |
| 204822807 | 0.364(2) | 0.096(9) | 2.06(3) | 0.01644(7) | 0.03914(9) | 0.0831(2) | 169.7(7) | 0.5, 0.4 |
| 204870619 | 0.528(4) | 0.05(2) | 0.0417(9) | 0.0403(2) | 0.0113(1) | 0.244(2) | 116.1(2) | 0.5, 0.7 |
| 205020466 | 0.79(1) | 0.03(2) | 0.74(2) | 0.0402(3) | 0.0390(4) | 0.34(1) | 143(2) | 2.8, 2.6 |
| 205170307 | 0.219(1) | 0.17(5) | 0.034(2) | 0.0193(2) | 0.0076(1) | 0.3282(8) | 162.0(5) | 0.3, 0.5 |
| 205546169 | 0.95(7) | 0.09(5) | 2.9(2) | 0.0193(3) | 0.0336(3) | 0.639(6) | 119.4(5) | 0.5, 0.3 |
| 205703649 | 0.94(2) | 0.8(2) | 1.2(4) | 0.071(5) | 0.081(5) | 0.004(2) | 310(34) | 0.8, 0.8 |
| 205919993 | 1.35(7) | =0 | =1.28(5) | 0.0269(5) | 0.0261(4) | 0.088(2) | 24(3) | 1.0, 0.9 |
| 205982900 | 0.929(3) | =0 | 1.329(6) | 0.0814(2) | 0.0974(1) | 0.1775(8) | 102.92(6) | 0.5, 0.4 |
| 206066862 | 0.36(6) | =0 | 0.20(5) | 0.040(2) | 0.029(2) | 0.205(8) | 152(4) | 1.2 |
| 206066909 | 0.189(2) | 0.52(2) | 0.0606(9) | 0.0420(3) | 0.0238(1) | 0.398(2) | 44.0(3) | 0.45 |
| 206084435 | 0.200(2) | 0.04(4) | 0.044(4) | 0.0189(2) | 0.0089(3) | 0.0896(2) | 177(2) | 1.0 |
| 206109641 | 0.932(3) | 0.0008(7) | 0.6664(9) | 0.01579(2) | 0.01336(1) | 0.63944(3) | 176.65(9) | 0.20 |
| 206212261 | 0.185(1) | 0.08(4) | 0.0169(6) | 0.0374(3) | 0.0113(1) | 0.085(2) | 297.1(6) | 0.3 |
| 206241558 | 1.6(1) | =0 | 0.6(1) | 0.0191(4) | 0.0120(5) | 0.587(4) | 135.6(7) | 0.8 |
| 206288770 | 0.0804(7) | 0.02(2) | 0.0138(2) | 0.0286(2) | 0.01186(8) | 0.345(3) | 35.6(8) | 0.4 |
| 206433263 | 0.691(3) | 0.008(7) | 0.188(1) | 0.03967(6) | 0.02072(6) | 0.098(1) | 252.8(2) | 0.4 |
Notes. Symbols used are defined in Sects. 2.4 and 2.5. The standard error in the final digit(s) of each parameter is given in parentheses. The standard error per observation as defined in Sect. 2.4 is given in the column σ in units of parts per thousand (ppt). For some light curves we give two values of σ because we assume different values of the standard error per observation for different parts of the light curve, as described in Sect. 2.4 Values preceded by “=” are either fixed or (if a standard error is given) imposed as constraints on the solution. See text for discussion of possible systematic errors in these parameters.
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