Table 1: Candidates with significant periodic variability (see text for explanations).
No. $M(M_{\odot})$ P(h) $\Delta P$(h) A(mag) FAP ${\rm _{E}}$(%) N
    4 0.17   56.1 2.33 0.027 <0.01 128
  17 0.05   9.46 0.14 0.027 <0.01 128
  20 0.08   35.2 0.98 0.034 <0.01 129
  24 0.22 100.0 10.5 0.023 <0.01 124
  26 0.27   18.0 0.47 0.037 <0.01 97
  28 0.21   96.8 8.50 0.042 <0.01 117
  29 0.27 100.4 11.3 0.027 <0.01 98
  39 0.06   19.2 0.34 0.038 <0.01 123
  44 0.12   31.0 1.78 0.027 <0.01 128
  45 0.09   14.6 0.42 0.022 <0.01 118
  51 0.16   15.7 0.51 0.073 <0.01 127
  56 0.12   33.7 1.09 0.030 <0.01 129
  60 0.12 102.1 11.6 0.017 <0.01 128
  61 0.18   40.1 0.72 0.069 <0.01 118
  63 0.04   15.5 0.31 0.426 <0.01 128
  65 0.02   4.70 0.08 0.049 <0.01 126
  69 0.12   3.80 0.05 0.020   0.01 112
  70 0.02   5.79 0.10 0.024 <0.01 127
  80 0.22   45.1 2.70 0.023 <0.01 127
  81 0.19   30.0 0.94 0.029 <0.01 125
  83 0.18   38.5 1.75 0.027 <0.01 115
  84 0.14   11.4 0.23 0.020 <0.01 127
  93 0.05   87.6 9.58 0.130 <0.01 129
110 0.11   35.9 2.31 0.025 <0.01 129
113 0.06   16.9 0.52 0.093 <0.01 125
118 0.19   98.0 4.85 0.089 <0.01 129
120 0.29   82.5 2.64 0.952 <0.01 129
123 0.05   34.3 1.32 0.037 <0.01 129
126 0.04   4.06 0.05 0.016 <0.01 128
132 0.11   32.3 1.84 0.022 <0.01 128


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Observations and image reduction
3 Photometry and astrometry
4 Target selection
5 Time series analysis
6 Origin of the variability - activity and accretion
7 Rotation periods
8 Conclusions
References
List of tables
List of figures