Table 1.
61 variables in our sample whose variability was attributed to rotation of the main sequence companion, identified by their TESS Input Catalogue (TIC) numbers.
| TIC | G | CROWDSAP | P (days) | Amplitude (%) | FAP |  (K) |
RMS (R⊙) |
|---|---|---|---|---|---|---|---|
| 3990402 | 11.08 | 0.98 | 3.5805(23) | 0.3169(23) | 0.00e+00 | 5794(78) | 1.14(6) |
| 12528447 | 12.50 | 1.00 | 0.67138(9) | 0.3340(46) | 0.00e+00 | 6720(163) | 1.61(6) |
| 16876025 | 12.86 | 1.00 | 2.326(7) | 0.205(8) | 0.00e+00 | 6172(73) | 1.27(7) |
| 30019744 | 12.12 | 0.71 | 2.113(11) | 0.163(7) | 0.00e+00 | 5758(25) | 1.57(6) |
| 32556882 | 13.82 | 0.80 | 5.35(5) | 0.454(28) | 0.00e+00 | 5328(20) | 1.221(50) |
| 33526769 | 12.24 | 0.99 | 2.2285(41) | 0.1467(36) | 0.00e+00 | 5531(42) | 0.986(40) |
| 64112207 | 15.32 | 0.99 | 7.26(16) | 0.252(40) | 5.39e−06 | 5772(75) | 2.10(26) |
| 65263746 | 13.40 | 0.78 | 4.498(28) | 0.171(10) | 6.49e−72 | 6146(117) | 0.82(7) |
| 68942649 | 10.04 | 0.98 | 2.8383(8) | 0.1954(10) | 0.00e+00 | 6400(400) | 1.10(5) |
| 69841801 | 12.25 | 1.00 | 1.251(17) | 0.88(14) | 0.00e+00 | 5896(41) | 1.398(48) |
| 70451188 | 14.22 | 0.99 | 2.836(14) | 0.305(19) | 0.00e+00 | 5965(24) | 1.28(6) |
| 71248239 | 12.83 | 0.89 | 0.9728(18) | 0.173(9) | 0.00e+00 | 6050(36) | 1.304(34) |
| 71716888 | 12.97 | 0.99 | 1.0491(23) | 0.066(29) | 3.75e–24 | 6992(39) | 1.62(8) |
| 92865531 | 13.12 | 0.96 | 1.40297(17) | 1.888(7) | 0.00e+00 | 5004(14) | 1.432(37) |
| 116416387 | 14.65 | 0.84 | 3.819(38) | 0.402(43) | 0.00e+00 | 5515(46) | 0.99(6) |
| 118269334 | 13.82 | 0.97 | 3.073(7) | 0.717(19) | 0.00e+00 | 5479(74) | 0.970(45) |
| 143058705 | 14.40 | 0.98 | 5.027(30) | 0.540(28) | 0.00e+00 | 5449(42) | 1.00(6) |
| 146323153 | 12.15 | 0.96 | 0.219040(20) | 0.1987(34) | 0.00e+00 | 6793(44) | 1.663(41) |
| 149767908 | 13.00 | 0.99 | 0.4557(6) | 0.229(10) | 0.00e+00 | 7300(56) | 1.67(12) |
| 151641733 | 12.65 | 0.96 | 0.5592(8) | 0.028(5) | 2.03e–10 | 6540(41) | 1.48(5) |
| 157323544 | 12.69 | 0.99 | 4.462(43) | 0.080(7) | 0.00e+00 | 6250(291) | 2.41(10) |
| 158335560 | 13.08 | 0.92 | 2.0007(41) | 0.244(13) | 0.00e+00 | 6063(71) | 1.45(8) |
| 159805154 | 14.80 | 0.90 | 2.686(9) | 0.29(34) | 5.95e–32 | 5642(50) | 1.50(23) |
| 160583519 | 14.43 | 0.98 | 1.9731(7) | 0.175(11) | 0.00e+00 | 5994(52) | 1.292(48) |
| 164754858 | 14.70 | 0.80 | 2.679(24) | 0.228(26) | 1.66e–11 | 5864(53) | 1.87(26) |
| 165650748 | 11.38 | 1.00 | 2.11600(19) | 0.0768(18) | 0.00e+00 | 6626(123) | 1.401(26) |
| 198240464 | 13.52 | 0.89 | 2.35724(7) | 0.816(6) | 0.00e+00 | 5646(53) | 1.195(23) |
| 202466623 | 13.81 | 0.97 | 3.3207(7) | 0.237(11) | 0.00e+00 | 6009(60) | 1.155(30) |
| 202507151 | 12.69 | 0.99 | 1.98289(36) | 0.135(5) | 0.00e+00 | 6356(69) | 1.032(27) |
| 206688085 | 13.77 | 0.99 | 1.91975(28) | 2.337(9) | 0.00e+00 | 4936(47) | 2.43(7) |
| 207208668 | 13.33 | 0.98 | 2.5671(6) | 0.36(36) | 0.00e+00 | 6111(52) | 1.166(37) |
| 209397773 | 12.73 | 0.83 | 3.58(9) | 0.08(5) | 1.05e–69 | 5460(34) | 1.230(40) |
| 212320065 | 11.64 | 0.98 | 1.8627(7) | 1.416(8) | 0.00e+00 | 5097(14) | 2.4992(9) |
| 219988867 | 13.03 | 0.96 | 1.9209(19) | 0.1007(39) | 0.00e+00 | 6093(57) | 1.446(38) |
| 228508601 | 14.40 | 0.99 | 5.58(6) | 0.346(24) | 0.00e+00 | 5400(41) | 1.97(33) |
| 231845752 | 13.72 | 0.96 | 2.0923(35) | 0.088(8) | 1.51e–31 | 5864(62) | 1.69(5) |
| 247017534 | 12.15 | 0.92 | 1.8154(46) | 0.09(10) | 0.00e+00 | 5945(28) | 1.355(49) |
| 263014094 | 15.03 | 0.88 | 2.91052(14) | 1.531(25) | 0.00e+00 | 5000(9) | 1.64(8) |
| 277892210 | 13.91 | 0.95 | 1.807791(24) | 1.658(28) | 0.00e+00 | 5460(49) | 1.234(32) |
| 293463617 | 15.13 | 0.87 | 1.74504(12) | 1.337(40) | 0.00e+00 | 4612(39) | 0.802(39) |
| 298093039 | 11.62 | 1.00 | 5.5610(6) | 0.1620(25) | 0.00e+00 | 5877(127) | 0.897(18) |
| 304103779 | 12.96 | 0.99 | 1.12766(11) | 0.0599(47) | 9.54e–37 | 5968(29) | 1.542(36) |
| 317129309 | 13.44 | 0.98 | 3.86(12) | 1.5(2.6) | 6.53e–24 | 6501(35) | 1.83(14) |
| 320529836 | 14.65 | 0.88 | 0.8353(8) | 1.84(13) | 0.00e+00 | 5251(44) | 0.969(45) |
| 320965274 | 12.66 | 0.99 | 1.759(6) | 0.0442(48) | 8.53e–22 | 5286(28) | 1.80(11) |
| 325566833 | 13.35 | 0.98 | 1.0628(15) | 0.069(7) | 9.39e–23 | 5291(22) | 1.283(19) |
| 335682563 | 13.55 | 0.99 | 4.4173(21) | 0.112(7) | 0.00e+00 | 5987(68) | 0.942(28) |
| 346597868 | 11.52 | 0.97 | 1.782(6) | 0.0320(34) | 5.51e–28 | 6438(97) | 2.29(7) |
| 349367583 | 13.05 | 0.99 | 2.302(14) | 0.23(24) | 0.00e+00 | 5919(53) | 1.465(49) |
| 365771053 | 13.37 | 0.85 | 1.3515(6) | 1.089(14) | 0.00e+00 | 5981(27) | 1.139(20) |
| 369371996 | 15.91 | 0.98 | 2.606(9) | 0.150(10) | 2.14e–40 | 5802(163) | 2.34(14) |
| 382518318 | 14.01 | 0.29 | 4.33102(40) | 1.402(25) | 0.00e+00 | 5206(25) | 1.274(36) |
| 389752750 | 15.24 | 0.82 | 0.67638(22) | 0.889(40) | 0.00e+00 | 4807(84) | 1.34(30) |
| 393941149 | 14.73 | 0.86 | 3.873(29) | 0.364(25) | 0.00e+00 | 5119(45) | 1.04(11) |
| 398940155 | 13.08 | 0.47 | 0.5039(7) | 0.62(12) | 0.00e+00 | 6976(65) | 2.10(14) |
| 405471275 | 15.19 | 0.33 | 3.510(40) | 0.42(6) | 2.66e–12 | 5915(56) | 1.29(29) |
| 406239686 | 13.45 | 0.98 | 1.633(5) | 0.12(13) | 1.16e–41 | 5499(32) | 1.395(46) |
| 420049852 | 12.13 | 0.81 | 1.666(7) | 0.0538(46) | 6.95e–35 | 6313(58) | 1.361(42) |
| 437237493 | 15.36 | 0.72 | 1.2648(39) | 0.84(42) | 0.00e+00 | 6186(60) | 1.41(19) |
| 441401311 | 13.74 | 0.99 | 2.915(6) | 0.275(12) | 0.00e+00 | 5741(21) | 1.46(7) |
| 461156754 | 14.96 | 0.74 | 1.610(6) | 0.321(42) | 2.32e–20 | 5730(59) | 1.57(17) |
Notes. G is the magnitude in the Gaia DR2 catalogue, and the value of CROWDSAP is the one calculated by the SPOC pipeline. For objects with data from more than one sector, this is the averaged value. Period and amplitude uncertainties were determined with a hundred Monte-Carlo runs of the multi-component fit to the light curve, re-drawing the fluxes from a normal distribution taking the quoted uncertainties into account. The FAP was calculated using the astropy LombScargle function. Teff and radius for the main sequence companion were obtained from a SED fit, as described in the text. Uncertainties are given on the last significant digits, e.g. 3.5805(23) = 3.5805 ± 0.0023, 1.5(2.6) = 1.5 ± 2.6, 6400(400) = 6400 ± 400.
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