Table 2: Photometric frequencies $f_{\rm 1}$-$f_{\rm 7}$ detected in analysis of entire data of the spectral order centered on 5825 Å. Also listed are the new modes detected in different subsets of the RV data.
No. Frequency K $\sigma _{K}$
  c d-1 $\mu $Hz m s-1  
Analysis of entire data set of $\lambda$ 5825Å order
$f_{\rm 1}$ 226.324 2619.5 20.1 (var) $\pm$0.6
$f_{\rm 2}^{-}$ 229.151 2652.2 18.6 $\pm$0.7
$f_{\rm 2}$ 229.206 2652.9 114.4 (var) $\pm$0.6
$f_{\rm 2}^{+}$ 229.294 2653.9 33.7 $\pm$0.7
$f_{\rm 3}$ 232.135 2687.6 53.9 (var) $\pm$0.6
$f_{\rm 4}$ 235.090 2720.9 88.4 (var) $\pm$0.6
$f_{\rm 4}^{-}$ 234.992 2719.8 37.3 $\pm$0.7
$f_{\rm 6}$ 241.29 2792.7 19.6 (var) $\pm$0.7
Analysis of subsets of the $\lambda$ 5825 Å spectral order
$f_{\rm 5}$ 238.09 2755.7 40.3 (var) $\pm$0.7
$f_{\rm 7}$ 242.41 2805.7 53.4 (var) $\pm$0.7
Analysis of subsets of the Nd III 5294.1 Å line
$f_{\rm -1}$ 220.58 2553.0 59.9 (var) $\pm$0.7
$f_{\rm0}$ 223.37 2585.3 50.3 (var) $\pm$0.7


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Observations and reduction
3 Time-series analysis
4 Discussion
5 Conclusions
References
List of tables
List of figures