1 Reinhold et al. (2015, J/A+A/583/A65) reports rotational period P.rot=17 day. The light curve shows rotationally modulated starspots with 0.1% amplitude. The TCF signals are weak and ARFIMA periodogram shows only the 1/2 times harmonic of the ARIMA peak, but RF-Prob is high.
 2 KOI 6282, classified as a False Positive, likely eclipsing binary, with P=88 days periodicity reported by Morton et al. (2016, J/ApJ/822/86); this signal is not found in the TCF periodogram. McQuillan et al. (2014, J/ApJS/211/24) reports rotational period P.rot=27 day. The light curve shows appearance and disappearance of rotationally modulated starspots with amplitudes 0.1-1%. Instrumental outlier with -1% amplitude at end of light curve has not been removed. ARPS finds strong TCF signals in both ARIMA and ARFIMA periodograms at this Ultrashort Period with with 2 times harmonic and clear transit-like dip in folded light curves.
 3 The identification LEDA 2115255 galaxy by Paturel et al. (2003, Cat. VII/237) seems incorrect. The light curve shows autocorrelation without obvious rotational modulation. The TCF peak is weak and folded light curves show transit-like dip with long duration.
 4 The light curve shows autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak but folded light curve dip has transit-like shape and RF-Prob is high.
 5 The light curve shows autocorrelation without obvious rotational modulation. The TCF periodogram peak is prominent with clear harmonics, and folded light curves show weak but transit-shaped dip.
 6 The light curve shows autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak but folded light curves show transit-like dip.
 7 The light curve shows autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak but folded light curves show clear transit-like dip.
 8 Tenenbaum et al. (2012, J/ApJS/199/24) reports possible planet with P=14.6 day and depth=432 ppm from Q1-Q3 data; this signal is now found in the TCF periodogram. The light curve shows autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak but folded light curves show a transit-like dip.
 9 The light curve shows rotational modulations of multiple short-lived spots with amplitudes <0.1%. The TCF shows clear peak with harmonic, and folded light curves show clear transit-like signal.
10 The light curve shows autocorrelation without obvious rotational modulation. Instrumental outlier with -1% amplitude at end of light curve has not been removed. The TCF periodogram peak is weak but folded light curve dip has transit-like shape.
11 A Kepler Threshold Crossing Event with possible period P=1.23 day periodicity is reported (Thompson et al. 2015, J/ApJ/812/46); this signal is not seen in the TCF periodogram. The light curve shows autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak but appears in both ARIMA and ARFIMA residuals with harmonic. The folded light curve has a strong transit-like dip and RF-Prob is high.
12 Strong rotationally modulated starspot with variable amplitude is present: Reinhold et al. (2015, J/A+A/583/A65) report P.rot=28.2-31.04 day with 0.8% variability range and McQuillan et al. (2014, J/ApJS/211/24) report P.rot=28.1 day with 0.6% range. Several positive outliers (flares) are not removed. The TCF periodogram peak is weak but the folded light curve has a clear transit-like dip and RF-Prob is high.
13 The light curve shows mild autocorrelation without obvious rotational modulation. The TCF periodogram peak is strong in both ARIMA and ARFIMA residuals with harmonic, the folded light curve has a clear transit-like dip, and the RF-Prob is very high.
14 The light curve shows mild autocorrelation without obvious rotational modulation. The TCF periodogram shows multiple weak peaks, possibly indicating multiple planets. The folded light curve has a transit-like dip.
15 The host is classified as a field star near open cluster NGC 6819 (Milliman et al. 2014, J/AJ/148/38). The light curve shows autocorrelation with confused rotational modulation. The TCF periodogram peak is weak but the folded light curve has a transit-like dip.
16 The light curve shows rotational modulation of multiple stars on a rapidly rotating star. Several positive outliers (flares) are not removed. TCF periodogram peak is weak but the folded light curve has a clear transit-like dip and RF-Prob is very high.
17 Tenenbaum et al. (2012, J/ApJS/199/24) reports a possible planet with P=15.0 day and depth=190 ppm from Q1-Q3 data; this signal is not seen in the TCF periodogram. The light curve shows mild autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak but the folded light curve has a transit-like dip with long duration and RF-Prob is high.
18 The host star is TYC 3125-567-1 with LAMOST spectral type F5V and rotational v(sini)=120 km/s (Frasca et al. 2016, J/A+A/594/A39). The light curve shows erratic weak variability with strong autocorrelation. The TCF periodogram peak is weak but the folded light curve has a transit-like dip and RF-Prob is high.
19 The host star is a radial velocity member of open cluster NGC 6819 (Platais et al. 2013, J/AJ/146/43). The light curve shows erratic variability with strong autocorrelation without obvious rotational modulation. The TCF periodogram peak is extremely strong with an UltraShort Period P=0.21 days and a full set of harmonics. The transit-shaped dip is strong in the folded light curves.
20 McQuillan et al. (2014, J/ApJS/211/24) report rotational modulation of starspots with P=1.61 day. Several positive outliers (flares) are not removed. The TCF periodogram peak is weak but the folded light curve has a transit-like dip.
21 Light curve shows autocorrelation without obvious rotational modulation. The TCF periodogram peak is strong with multiple harmonics. A transit-shaped dip with long duration is present in the folded light curves.
22 The light curve shows autocorrelation without obvious rotational modulation. Both the TCF periodogram peak and folded light curve dip are weak, but the RF-Prob is high.
23 The light curve shows autocorrelation without obvious rotational modulation. The TCF periodogram peak i strong in both the ARIMA and ARFIMA residuals, a transit-like dip spanning a large fraction of this UltraShort Period orbit in the folded light curve dip are weak, and the RF-Prob is high.
24 Lightcurve shows strong autocorrelation from rotational modulation of multiple starspots with amplitude around 0.4%. The TCF periodogram peak is clearly present with a harmonic, and an obvious transit-like dip is present in the folded light curves.
25 The light curve shows autocorrelation without obvious rotational modulation. The TCF periodogram peak and transit-like dip in the folded light curves are clearly present, and RF-Prob is high.
26 KOI 4305, this star is reported as a False Positive periodic variable with P=0.94 day and depth 71 ppm classified by Coughlin et al. (2014, J/AJ/147/119) and Rowe et al. (2015, J/ApJS/217/16). This is the 4 times harmonic of the UltraShort Period P=0.234 day reported here. A transit-shaped dip is clearly present in the folded light curve.
27 The light curve shows strong autocorrelation without obvious rotational modulation. A strong TCF periodogram with harmonics is present, along with other peaks suggesting multiple planets. The folded light curves are somewhat noisy, and RF-Prob is high.
28 The light curve shows strong autocorrelation without obvious rotational modulation and occasional appearance of large starspots. The TCF periodogram peak is weak, but the folded light curve show a short-duration transit-shaped dip harmonics is present, along with other peaks suggesting multiple planets. The folded light curves are somewhat noisy, and RF-Prob is high.
29 The host star is a giant with LAMOST spectral type K4-G3 III (Gray et al. 2016, J/AJ/151/13). McQuillan et al. (2014, J/ApJS/211/24) report a rotation period P.rot=60 day. The light curve is strongly autocorrelated with indications of multiple starspots. The TCF peak is weak but the folded lighturve shows a transit-like dip.
30 The light curve shows mild autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak but the folded light curve has a clear transit-like dip and RF-Prob is high.
31 The light curve is quiet with weak autocorrelation and without obvious rotational modulation. The TCF periodogram peak is present in both ARIMA and ARFIMA residuals but without evident harmonics. The folded light curve has a broad transit-like dip with an UltraShort Period.
32 The light curve shows strong autocorrelation without obvious rotational modulation. The TCF periodogram peak is clear with harmonic although other short-period peaks are present. The folded light curve has a faint broad transit-like dip with an UltraShort Period.
33 Light curve shows strong autocorrelation from rotational modulated starspots. The TCF periodogram peak is clear in both ARIMA and ARFIMA residuals with harmonic. The folded light curve has a transit-like dip with an UltraShort Period and RF-Prob is high.
34 The light curve is quiet with mild autocorrelation. The TCF periodogram peak is weak without harmonics. The folded light curve has a clear transit-like dip and RF-Prob is high.
35 The light curve has low-level erratic variability with strong autocorrelation. The TCF periodogram peak is clear without harmonics. The folded light curve has a clear transit-like dip and RF-Prob is very high.
36 The light curve shows strong autocorrelation from rotationally modulated starspots. The TCF periodogram peak is present in ARIMA and ARFIMA residuals without harmonics. The folded light curve has a transit-like dip and RF-Prob is very high.
37 The light curve shows strong autocorrelation without obvious rotational modulation. The TCF periodogram peak is very strong in ARIMA and ARFIMA residuals with harmonics. The folded light curve has a transit-like dip with an UltraShort Period.
38 The light curve shows strong autocorrelation from rotational modulation of multiple starspots. The TCF periodogram peak is strong but without harmonics. The folded light curve has a weak transit-like dip.
39 KOI 4777 with  period P=0.82 day; this is the 2 times harmonic of the TCF period. The NASA Exoplanet Archive gives disposition CANDIDATE, but Morton et al. (2016, J/ApJ/822/86) gives disposition False Positive due to possible background eclipsing binary. The light curve shows erratic, strong variability from rotationally modulated starspots. The TCF periodogram peak is strong with P=0.412 days in ARIMA and ARFIMA residuals with harmonics. The folded light curve has a clear transit-like dip and RF-Prob is very high.
40 The light curve shows strong autocorrelation from rotationally modulated starspots. The TCF periodogram peak is weak and alternative peaks (P~0.7 and 38.7 days) may represent true periodicities. The folded light curve has a clear transit-like dip.
41 KOI 6749 with periodicity P=18.36 day, the same as the TCF period. Morton et al. (2016, J/ApJ/822/86) disposition False Positive as a possible unblended eclipsing binary. The light curve shows strong autocorrelation from erratic variability due to rotationally modulated starspots. The TCF periodogram peak is weak with a long period. The folded light curve has a weak transit-like dip and RF-Prob is high.
42 The light curve shows strong autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak without harmonics. The folded light curve shows a clear transit-like dip and RF-Prob is high.
43 The light curve shows strong autocorrelation from rotational modulated starspots. The TCF periodogram peak is weak.  The folded light curve shows a weak transit-like dip and RF-Prob is very high.
44 The light curve is quite with mild autocorrelation. The TCF periodogram peak is clear without harmonics. The folded light curve shows a transit-like dip and RF-Prob is very high.
45 The light curve shows strong autocorrelation and erratic variability from rotationally modulated starspots with short-memory volatility. The TCF periodogram peak is clear without harmonics. The folded light curve shows a transit-like dip.
46 Reinhold et al. (2013, J/A+A/560/A4) report a rotational period=18.7/23.4 d with variability range 0.3%. The light curve shows strong autocorrelation from rotational modulation of multiple starspots. The TCF periodogram peak is weak. The folded light curve shows a transit-like dip.
47 The light curve shows strong autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak but exhibits a harmonic. The folded light curve shows a transit-like dip with an UltraShort period.
48 The light curve is quiet with weak autocorrelation. The TCF periodogram peak is strong with harmonics. The folded light curve shows a weak transit-like dip and the RF-Prob is very high.
49 The light curve shows some autocorrelation without obvious rotational modulation. The TCF periodogram peak is strong. The folded light curve shows a transit-like dip.
50 The light curve is quiet with low autocorrelation. An instrumental outlier at the end of the time series has not been removed. The TCF periodogram peak is weak without harmonics. The folded light curve shows a transit-like dip.
51 The light curve shows strong autocorrelation from rotational modulated starspots. The TCF periodogram peak is weak. The folded light curve shows a clear transit-like dip.
52 Frasca et al. (2016, J/A+A/594/A39) report a LAMOST spectral type of K1 III or G6 V. The light curve shows erratic low-amplitude autocorrelated variations. The TCF periodogram peak is very strong in ARIMA and ARFIMA residuals with harmonic. The folded light curve shows a transit-like dip, and the RF-Prob is very high.
53 The light curve shows volatile variability from rotationally modulated starspots: Reinhold et al. (2015, J/A+A/583/A65) report P~22.1-27.2 day and McQuillen et al. (2014, J/ApJS/211/24) report P=24.6 day with range 0.5%. The TCF periodogram peak is strong without harmonic. The TCF shows a transit-like dip and the RF-Prob is high.
54 The light curve shows mild autocorrelation without obvious rotational modulation. The TCF periodogram peak has moderate intensity. The folded light curve shows a weak transit-like dip.
55 McQuillen et al. (2014, J/ApJS/211/24) report rotational P=35.1 day with range 0.3%. The light curve shows volatile rotational modulation of multiple starspots. The TCF periodogram peak is moderately strong with harmonic. The folded light curve shows a transit-like dip and the RF-Prob is high.
56 The light curve is quiet with mild autocorrelation. A strong positive outlier is present and other weaker outliers (flares?) may be present. The TCF is noisy at long periods, but the peak at P=3.67 days is relatively strong and isolated. The folded light curve shows a transit-like dip.
57 The light curve shows strong strong autocorrelation from rotational modulated starspots. The TCF periodogram peak is not strong but appears in both ARIMA and ARFIMA residuals. The folded light curve shows a transit-like dip.
58 The light curve shows weak, but volatile, autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak without harmonic. The folded light curve shows a clear transit-like dip.
59 The light curve shows strong autocorrelation without obvious rotational modulation. The TCF periodogram peak is strong with harmonic. The folded light curve shows a weak transit-like dip and RF-Prob is high.
60 The light curve shows strong autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak without harmonic. The folded light curve shows a clear transit-like dip.
61 The light curve shows strong variations from rotationally modulated starspots: Nielsen et al. (2013, J/A+A/557/L10) report P=9.0 day, McQuillen et al. (2014, J/ApJS/211/24) report P=9.0 day with range 1.0%, and Reinhold et al. (2015, J/A+A/583/A65) report P=8.9-9.4 day with range 1.3%. The TCF periodogram peak is very strong with harmonic; other short-period planetary signals may be present. The folded light curve shows a weak transit-like dip.
62 The light curve shows moderate autocorrelation without obvious rotational modulation. The TCF periodogram peak is moderately strong without harmonic. The folded light curve shows a weak transit-like dip and RF-Prob is high.
63 The light curve shows strong variations from rotationally modulated starspots: Nielsen et al. (2013, J/A+A/557/L10) report P=9.6 day, McQuillen et al. (2014, J/ApJS/211/24) report P=9.2 day with range 0.5%, and Reinhold et al. (2015, J/A+A/583/A65) report P=8.9-9.4 day with range 1.3%. The TCF periodogram peak is moderately strong with harmonic. The folded light curve shows a weak transit-like dip.
64 KOI 6984 with period P=1.02 day classified as False Positive with a low probability as a background eclipsing binary by Morton et al. (2016, J/ApJ/822/86); this is the TCF peak period. Light curve is quiet with mild autocorrelation and possible weak flare outliers. The TCF periodogram peak is extremely strong with harmonics. The folded light curve shows a clear transit-like dip.
65 This star is a likely member of open cluster NGC 6866 (Joshi et al. 2012, J/MNRAS/419/2379). The light curve shows moderate autocorrelation without obvious rotational modulation. The TCF periodogram peak is moderately strong; the 2 times harmonic at P=1.91 day has comparable strength. The folded light curve shows a weak transit-like dip.
66 The light curve shows moderate autocorrelation without obvious rotational modulation. Two positive outliers (flares?) have not been removed.  The TCF periodogram peak is moderately strong with harmonic. The folded light curve shows a clear transit-like dip.
67 Frasca et al. (2016, J/A+A/594/A39) report LAMOST spectral type F3 V. The light curve shows short-memory autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak without harmonic. The folded light curve shows an extremely clear transit-like dip.
68 Frasca et al. (2016, J/A+A/594/A39) report LAMOST spectral type F3-F5 V. The light curve is shows moderate autocorrelation without obvious rotational modulation. The TCF periodogram peak is very strong in ARIMA and ARFIMA residuals with harmonics. The folded light curve shows an extremely clear transit-like dip and RF-Prob is high.
69 The light curve shows strong short-memory autocorrelation without obvious rotational modulation. The TCF periodogram peak is very strong without harmonic; additional planetary signals may be present. The folded light curve shows an extremely clear transit-like dip and RF-Prob is high (Figure 12 here).
70 KOI 5547. This KOI is classified as "Candidate" with P=571 day in the NASA Exoplanet Archive, does not appear as a KOI in the MAST archive, and is not classified as False Positive by Mazeh et al. (2015, J/ApJ/801/3). The light curve shows highly volatile rotationally modulated starspots; Reinhold et al. (2013, J/A+A/560/A4) report P=28.7 day and McQuillen et al. (2014, J/ApJS/211/24) report P=21.6 day with 0.4% amplitude. The TCF periodogram peak is weak without harmonic. The folded light curve shows a transit-like dip.
71 The light curve shows moderate autocorrelation without obvious rotational modulation. The TCF periodogram peak  is weak without harmonic. The folded light curve shows a weak transit-like dip.
72 Luo et al. (2016, Cat. V/149) report LAMOST spectral type G0. The light curve shows strong autocorrelation without obvious rotational modulation. The TCF periodogram peak is clearly present without harmonic. The folded light curve shows a transit-like dip.
73 Frasca et al. (2016, J/A+A/594/A39) report LAMOST spectral type K0 V. The light curve is quiet with weak autocorrelation. The TCF periodogram peak is present without harmonic. The folded light curve shows a clear transit-like dip and RF-Prob is very high.
74 Frasca et al. (2016, J/A+A/594/A39) report LAMOST spectral type F6 IV. The light curve is shows strong autocorrelation without obvious rotational modulation. A positive outlier (flare?) has not been removed. The TCF periodogram peak is very strong in ARIMA and ARFIMA residuals with harmonic. The folded light curve shows a faint transit-like dip.
75 KOI 2341 classified as False Positive (Rowe et al. 2015, J/ApJS/217/16). Coughlin et al. (2014, J/AJ/147/119) report a periodicity with P=0.99 day and depth 159 ppm; this signal is not present in the TCF periodogram. The light curve is quiet with weak autocorrelation. The TCF periodogram peak is very strong in ARIMA and ARFIMA residuals with harmonics. Other planetary transit signals may be present. The folded light curve shows an extremely clear transit-like dip and RF-Prob is very high.
76 Reinhold et a. (2013, J/A+A/560/A4) report rotational period P= 27.8 day  with variability range 0.7%. The light curve shows strong autocorrelation from rotationally modulated starspots. The TCF periodogram peak is weak without harmonic. The folded light curve shows a transit-like dip.
77 The light curve shows strong autocorrelation with rotational modulation of multiple starspots. The TCF periodogram peak is very strong in ARIMA and ARFIMA residuals with harmonics. The folded light curve shows a clear transit-like dip and RF-Prob is high.
78 The light curve shows strong autocorrelation with rotational modulation of multiple starspots. The TCF periodogram peak is weak without harmonics. The folded light curve shows a transit-like dip.
79 The light curve shows strong autocorrelation with rotationally modulated multiple starspots. The TCF periodogram peak is extremely strong in ARIMA and ARFIMA residuals with harmonics. The folded light curve clearly shows a transit-like dip.
80 The light curve shows weak autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak without harmonics. The folded light curve clearly shows a transit-like dip.
81 The light curve is quiet with weak autocorrelation. A high-amplitude outlier (instrumental origin?) has not been removed; this produces periodogram noise at long periods. The TCF periodogram peak is moderately strong in ARIMA and ARFIMA residuals weak without harmonics. The folded light curve clearly shows a transit-like dip.
82 The light curve is quiet with weak autocorrelation. The TCF periodogram peak is very strong in ARIMA and ARFIMA residuals weak with harmonic. The folded light curve shows a clear transit-like dip and RF-Prob is high.
83 KOI 4788, periodicity P=2.18 day with depth 74 ppm, classified as False Positive (Rowe et al. 2015, J/ApJS/217/16). This is the 2 times harmonic of the TCF period. Morton et al. (2016, J/ApJ/822/86) disposition is False Positive due to possible background eclipsing binary. The light curve is quiet with weak autocorrelation. The TCF periodogram peak is weak with harmonic. The folded light curve shows a weak transit-like dip and RF-Prob is very high.
84 The light curve is highly volatile with a brief period exhibiting a large rotationally modulated starspot. Some quarters are missing from the light curve. The TCF periodogram peak is weak in ARIMA and ARFIMA residuals weak without harmonics. The folded light curve shows a transit-like dip and RF-Prob is high.
85 Frasca et al. (2016, J/A+A/594/A39) reports LAMOST spectral type G2 V. The light curve shows strong autocorrelation with rotational modulation of multiple starspots. The TCF periodogram peak is extremely strong in ARIMA and ARFIMA residuals with harmonics. Additional planetary signals are probably present. The folded light curve clearly shows a transit-like dip.
86 The light curve shows strong autocorrelation with rotational modulation of multiple starspots. Rotational period is reported to be P=19.6 day with variability range 1.1% by Reinhold et al. (2013, J/A+A/560/A4), 19.4 day with range 1.1% by McQuillan et al. (2014, J/ApJS/211/24), and 19.7-20.7 day by Reinhold et al. (2015, J/A+A/583/A65). The TCF periodogram peak is weak without harmonics. The folded light curve shows a transit-like dip.
87 The light curve is quiet with weak autocorrelation. The TCF periodogram peak is moderately weak without harmonic. The folded light curve shows a clear transit-like dip.
88 The light curve shows strong autocorrelation with rotational modulation of multiple starspots. The TCF periodogram peak is weak with harmonic. The folded light curve shows a clear transit-like dip.
89 This star is identified as a UltraShort Period "new planet candidate" with P=0.305 day by Sanchis-Ojeda et al. (2014, J/ApJ/787/47). The light curve is quiet with weak autocorrelation. The TCF periodogram peak is extremely strong with harmonics. Additional planetary transit signals may be present. The folded light curve shows a strong transit-like dip and RF-Prob is very high.
90 KOI 4872. This star is identified be the Kepler team as a Planet Candidate with period P=1.035 day (Rowe et al. 2015, J/ApJS/217/16); this is the 5 times harmonic of the TCF period. The light curve shows moderate autocorrelation with volatility. The TCF periodogram peak is extremely strong with harmonics. The folded light curve shows a very strong transit-like dip and RF-Prob is high.
91 The light curve shows strong autocorrelation with rotational modulation of multiple starspots. The TCF periodogram peak is weak without harmonic. The folded light curve shows a clear transit-like dip.
92 The light curve shows moderate autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak without harmonic. The folded light curve shows a transit-like dip and RF-Prob is very high.
93 The light curve shows strong autocorrelation with rotational modulation of multiple starspots. The TCF periodogram peak is strong with harmonic. The folded light curve shows a weak transit-like dip and RF-Prob is high.
94 The light curve shows weak autocorrelation. Three outliers (instrumental origin?) are not removed. The TCF periodogram peak is moderately strong in the ARIMA and ARFIMA residuals without harmonic. The folded light curve shows a weak transit-like dip.
95 KOI 2642 designated by the Kepler team as a False Positive (Rowe et al. 2015, J/ApJS/217/16). The light curve shows weak autocorrelation. The TCF periodogram peak is very strong in the ARIMA and ARFIMA residuals with harmonic. Additional planetary signals may be present. The folded light curve shows a strong k transit-like dip and RF-Prob is very high.
96 The light curve shows moderate autocorrelation without obvious rotational modulation. The TCF periodogram peak is moderately strong without harmonic. The folded light curve shows a weak transit-like dip and RF-Prob is very high.
97 The light curve shows weak autocorrelation without obvious rotational modulation. The TCF periodogram peak is weak without harmonic. The folded light curve shows a weak transit-like dip and RF-Prob is high.