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Table 3.

Photometric periods from BRITE.

Name Satellite rmsall P ΔP FAP Amp T0 rmsfit
(mmag) (d) (d) (−) (mmag) (TJD) (mmag)
α Aur BTr 1.02 4.38 0.11 0.014 0.36 1813.1686 1.01
BLb 0.96 10.1018 0.57 0.0001 0.89 1803.9445 0.90
β Aur BTr 18.06 3.9601 0.0001 <10−20 82.06 1816.9535 2.80
BLb 16.17 3.9601 0.0001 <10−20 81.24 1816.9535 1.87
ε Aur BTr 31.05 152.661 0.064 <10−20 121.68 1515.3200 4.78
BLb 28.58 ... ... ... ... ... ...
ζ Aur BTr 26.83 69.949 0.037 <10−20 95.72 1659.2235 9.52
BLb 41.70 ... ... ... ... ... ...
η Aur BTr 5.05 1.2891 0.0001 <10−20 7.34 1819.8943 4.34
BLb 8.54 1.2777 0.0014 2.09 × 10−18 10.99 1819.8943 7.56
θ Aur BTr 12.30 3.6189 0.0001 <10−20 34.71 1817.6543 1.24
BLb 12.19 3.6192 0.0002 <10−20 34.02 1817.6543 2.66
ν Aur BTr 2.71 19.159 0.085 2.86 × 10−12 1.81 1795.7694 2.66
ι Aur BTr 3.14 9.0712 0.0019 <10−20 4.27 1800.6762 2.80
BLb 5.11 ... ... ... ... ... ...
β Tau BTr 5.37 ... ... ... ... ... ...
BLb1 1.78 2.7371 0.0044 0.19 ... ... ...
BLb2 1.78 2.7414 0.0028 0.0069 0.54 2868.7218 1.16
κ1 Cet BHr 4.31 9.0648 0.018 <10−20 12.76 1744.8921 2.72
V711 Tau BHr 26.68 2.8359 0.0003 <10−20 79.95 1751.8432 4.77
IQ Aur BTr 11.08 2.4630 0.0092 2.56 × 10−5 20.13 1694.1688 9.31

Notes. Column rmsall is the standard deviation from the entire data set and just indicates the level of photometric variability in the respective satellite bandpass (BTr and BHr are red sensitive, BLb is blue sensitive). Column ΔP is the error from a Monte Carlo simulation of 10 000 synthetic data sets. Column Amp is the peak-to-valley amplitude and T0 is the phase zero point in heliocentric truncated Julian days (HJD = TJD + 2 456 000). Column rmsfit is the rms of the data after removal of the (multi)harmonic fit.

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