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Observations Summary

Instrument
 		 #Meas
 		 T*min
[day]		 T*max
[day]		 ΔT
[day]		 RV
[m/s]		 RVerr
[m/s]		 FeH
 		 Vsini
[km/s]

T* = bjd - 2,400,000
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ParameterFromToFromTo
RJD (ex: 54000.0)
RV [m/s]
RV Error [m/s]
FWHM [m/s]
BIS [m/s]
Contrast [m/s]
S-Index [-]
Hα-Index [-]
Na-Index [-]
Log(R'/HK) [-]
Berv [m/s]
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Correlations


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Z: 
Residuals




Correlations:

R : 0.0
Weighted R : 0.0







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    From [BJD -2,450,000.0]:
    To [BJD -2,450,000.0]:
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  • False Alarm Probability

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Star barycentric orbit

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Relative orbits
Acknowledgements Keplerian model initial conditions are computed using the formalism described in Delisle et al. 2016. Activity cycles are modeled following Delisle et al. 2018. Analytical FAP values are estimated following Baluev 2008, and numerical FAP values are computed by permutation of the calendar. The MCMC algorithm is described in Díaz et al. 2014, 2016. References