Fit

Data Reduction Products Download (Fits)

Instrument Selected Data All Data

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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Pre-binningPost-binning
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]
DRS quality control:

Correlations


X: 
Y: 

Z: 
Residuals




Correlations:

R : 0.0
Weighted R : 0.0







Data Binning:     




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auto




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Star barycentric orbit
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